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APOKASC-3: The Third Joint Spectroscopic and Asteroseismic catalog for Evolved Stars in the Kepler Fields
Volume 19, Issue 40 - article #1
Marc H. Pinsonneault
(Department of Astronomy, The Ohio State University, USA),
Joel C. Zinn
(Department of Physics, California State Long Beach, USA),
Jamie Tayar
(Department of Astronomy, University of Florida, USA),
Aldo Serenelli
(Institute of Space Sciences, ICE, CSIC, Spain, Institut d'Estudis Espacials de Catalunya, Spain),
Rafael A. Garcia
(Universite Paris Cite, CEA, CNRS, France),
Savita Mathur
(Instituto de Astrofsica de Canarias, Spain, Departamento de Astrofisica Universidad de La Laguna, Spain, Space Science Institute, USA),
Mathieu Vrard
(Department of Astronomy, The Ohio State University, USA, Observatoire de la Cote d'Azur CNRS, France),
Yvonne P. Elsworth
(School of Physics, Astronomy, University of Birmingham, UK, Stellar Astrophysics Centre, Department of Physics, Astronomy, Aarhus University, Denmark),
Benoit Mosser
(LESIA Observatoire de Paris Universite, PSL, CNRS, Sorbonne Universite, Universite de Paris, France),
Dennis Stello
(School of Physics, University of New South Wales, Australia, Sydney Institute for Astronomy, School of Physics, University of Sydney, Australia, ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions, Australia),
Keaton J. Bell
(Department of Physics, Queens College, CUNY, USA),
Lisa Bugnet
(Institute of Science, Technology Austria),
Enrico Corsaro
(INAF, Osservatorio Astrofisico di Catania, Italy),
Patrick Gaulme
(Thuringer Landessternwarte, Germany, Department of Astronomy, New Mexico State University, USA),
Saskia Hekker
(Stellar Astrophysics Centre, Department of Physics, Astronomy, Aarhus University, Denmark, Heidelberg University, Germany, Heidelberg Institute for Theoretical Studies, Germany),
Marc Hon
(Kavli Institute for Astrophysics, Space Research, Massachusetts Institute of Technology, USA, Institute for Astronomy, University of Hawaii, USA),
Daniel Huber
(Institute for Astronomy, University of Hawaii, USA, SIfA, School of Physics, University of Sydney, Australia),
Thomas Kallinger
(Institute for Astronomy, University of Vienna, Austria),
Kaili Cao
(Center for Cosmology, AstroParticle Physics, Department of Physics, The Ohio State University, USA),
Jennifer A. Johnson
(Department of Astronomy, The Ohio State University, USA, Center for Cosmology, AstroParticle Physics),
Bastien Liagre
(Universite Paris Cite, CEA, CNRS, France, Instituto de Astrofsica de Canarias, Spain, ENS Paris-Saclay, Universite Paris-Saclay, France),
Rachel A. Patton
(Department of Astronomy, The Ohio State University, USA, Center for Cosmology, AstroParticle Physics),
Angela R. G. Santos
(Instituto de Astrofisica e Ciencias do Espac{c}o, Universidade do Porto, Portugal),
Sarbani Basu
(Department of Astronomy, Yale University, USA),
Paul G. Beck
(Instituto de Astrofsica de Canarias, Spain, Departamento de Astrofisica Universidad de La Laguna, Spain),
Timothy C. Beers
(Dept. of Physics, Astronomy,, JINA Center for the Evolution of the Elements University of Notre Dame, USA),
William J. Chaplin
(School of Physics, Astronomy, University of Birmingham, UK, Stellar Astrophysics Centre, Department of Physics, Astronomy, Aarhus University, Denmark),
Katia Cunha
(University of Arizona, Steward Observatory, USA, Observatorio Nacional, Sao Cristovao, Brazil),
Peter M. Frinchaboy
(Department of Physics, Astronomy, Texas Christian University, USA, Maunakea Spectroscopic Explorer, Canada-France-Hawaii-Telescope, USA),
Leo Girardi
(Osservatorio Astronomico di Padova, INAF, Italy),
Diego Godoy-Rivera
(Instituto de Astrofsica de Canarias, Spain, Departamento de Astrofisica Universidad de La Laguna, Spain),
Jon A. Holtzman
(Department of Astronomy, New Mexico State University, USA),
Henrik Jonsson
(Materials Science, Applied Mathematics, Malmo University, Sweden),
Szabolcs Meszaros
(ELTE Eotvos Lorand University, Gothard Astrophysical Observatory, Hungary, MTA-ELTE Lendulet Momentum Milky Way Research Group, Hungary),
Claudia Reyes
(School of Physics, University of New South Wales, Australia),
Hans-Walter Rix
(Max Planck Institute for Astronomy, Heidelberg, Germany),
Matthew Shetrone
(University of California Observatories, University of California Santa Cruz, USA),
Verne V. Smith
(NSFs NOIRLab, USA),
Taylor Spoo
(Department of Physics, Astronomy, Texas Christian University, USA),
Keivan G. Stassun
(Department of Physics, Astronomy, Vanderbilt University, USA),
Ji Wang
(Department of Astronomy, The Ohio State University, USA)
https://arxiv.org/abs/2410.00102
The accretion history of the Milky Way IV. Hints of recent star formation in Milky Way dwarf spheroidal galaxies
Volume 19, Issue 39 - article #6
Yanbin Yang
(GEPI, Observatoire de Paris, Universite PSL, CNRS, Meudon, France),
Elisabetta Caffau
(GEPI, Observatoire de Paris, Universite PSL, CNRS, Meudon, France),
Piercarlo Bonifacio
(GEPI, Observatoire de Paris, Universite PSL, CNRS, Meudon, France),
Franc{c}ois Hammer
(GEPI, Observatoire de Paris, Universite PSL, CNRS, Meudon, France),
Jianling Wang
(CAS Key Laboratory of Optical Astronomy, National Astronomical Observatories, Beijing, China),
Gary A. Mamon
(Institut v{d}Astrophysique de Paris)
https://arxiv.org/abs/2409.15414
Supernova Simulations
Volume 19, Issue 13 - article #5
Bernhard M"uller
(School of Physics,Astronomy, Monash University)
https://arxiv.org/abs/2403.18952
SkyMapper Southern Survey: Data Release 4
Volume 19, Issue 6 - article #5
Christopher A. OnkenResearch School of Astronomy
,
Astrophysics
,
Australian National University
,
Centre for Gravitational Astrophysics
,
Australian National University Christian WolfResearch School of Astronomy
,
Astrophysics
,
Australian National University
,
Centre for Gravitational Astrophysics
,
Australian National University Michael S. BessellResearch School of Astronomy
,
Astrophysics
,
Australian National University Seo-Won ChangAstronomy Program
,
Department of Physics
,
Astronomy
,
Seoul National University
,
SNU Astronomy Research Center
,
Seoul National University Lance C. LuvaulResearch School of Astronomy
,
Astrophysics
,
Australian National University John L. TonryInstitute for Astronomy
,
University of Hawaii Marc C. WhiteResearch School of Astronomy
,
Astrophysics
,
Australian National University Gary S. Da CostaResearch School of Astronomy
,
Astrophysics
,
Australian National University
https://arxiv.org/abs/2402.02015
Gaia EDR3 proper motions, energies, angular momenta of Milky Way dwarf galaxies: a recent infall to the Milky Way halo. (arXiv:2306.17208v1 [astro-ph.GA])
Volume 18, Issue 27 - article #2
Yang Y.
(1),
Hammer F.
(1),
Li H.
(2),
Pawlowski M. S.
(3),
Wang J. L.
(4),
Babusiaux C.
(5),
Mamon G. A.
(6),
Bonifacio P.
(1),
Jiao Y.
(1),
Wang H.
(7)
((1) Observatoire de Paris, Paris Sciences et Lettres, CNRS France,
(2) School of Physical Sciences, University of Chinese Academy of Sciences, Beijing, China,
(3) Leibniz-Institut fuer Astrophysik Potsdam, Germany,
(4) CAS Key Laboratory of Optical Astronomy, National Astronomical Observatories, Beijing 100101, China,
(5) Université de Grenoble-Alpes, CNRS, IPAG, F-38000 Grenoble, France,
(6) Institut d'Astrophysique de Paris, CNRS, France,
(7) Centro Ricerche Enrico Fermi, Roma, Italy)
http://arxiv.org/abs/2306.17208
Predicting light curves of RR Lyrae variables using artificial neural network based interpolation of a grid of pulsation models. (arXiv:2303.15117v1 [astro-ph.SR])
Volume 18, Issue 13 - article #7
Nitesh Kumar
(1),
Anupam Bhardwaj
(2),
Harinder P. Singh
(1),
Susmita Das
(3),
Marcella Marconi
(2),
Shashi M. Kanbur
(4),
Philippe Prugniel
(5)
((1) Department of Physics, Astrophysics, University of Delhi, Delhi 110007, India
(2) INAF-Osservatorio Astronomico di Capodimonte, Salita Moiariello 16, 80131, Naples, Italy
(3) Konkoly Observatory, Research Centre for Astronomy, Earth Sciences, Eötvös Loránd Research Network
(ELKH), Konkoly-Thege Miklós út 15-17, H-1121, Budapest, Hungary
(4) Department of Physics, Earth Science, State University of New york at Oswego, Oswego, NY 13126, USA
(5) Université de Lyon, Université Lyon 1, 69622 Villeurbanne, CRAL, Observatoire de Lyon, CNRS UMR 5574, 69561 Saint-Genis Laval, France)
http://arxiv.org/abs/2303.15117
RR Lyrae mid-infrared Period-Luminosity-Metallicity and Period-Wesenheit-Metallicity relations based on Gaia DR3 parallaxes. (arXiv:2301.03777v1 [astro-ph.GA])
Volume 18, Issue 2 - article #2
Joseph P. Mullen
(1),
Massimo Marengo
(1, 2),
Clara E. Martínez-Vázquez
(3, 4),
Brian Chaboyer
(5),
Giuseppe Bono
(6, 7),
Vittorio F. Braga
(7, 8),
Massimo Dall'Ora
(9),
Valentina D'Orazi
(6, 10),
Michele Fabrizio
(7, 11),
Matteo Monelli
(8, 12),
Frédéric Thévenin
(13)
((1) Department of Physics, Astronomy, Iowa State University, Ames, IA, USA,
(2) Department of Physics, Florida State University, Tallahassee, FL, USA,
(3) Gemini Observatory, NSF's National Optical-Infrared Astronomy Research Laboratory, Hilo, HI, USA,
(4) Cerro Tololo Inter-American Observatory, NSF's National Optical-Infrared Astronomy Research Laboratory, La Serena, Chile,
(5) Department of Physics, Astronomy, Dartmouth College, Hanover, NH, USA,
(6) Dipartimento di Fisica, Università di Roma Tor Vergata, Roma, Italy,
(7) INAF-Osservatorio Astronomico di Roma, Monte Porzio Catone, Italy,
(8) Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain,
(9) INAF-Osservatorio Astronomico di Capodimonte, Napoli, Italy,
(10) INAF-Osservatorio Astronomico di Padova, Padova, Italy,
(11) Space Science Data Center, Roma, Italy,
(12) Departmento de Astrofísica, Universidad de La Laguna, La Laguna, Tenerife, Spain,
(13) Université de Nice Sophia-antipolis, CNRS, Observatoire de la Côte d'Azur, Laboratoire Lagrange, Nice, France)
http://arxiv.org/abs/2301.03777
The Galactic Chemical Evolution of phosphorus observed with IGRINS. (arXiv:2210.04940v1 [astro-ph.SR])
Volume 17, Issue 40 - article #10
G. Nandakumar
(1),
N. Ryde
(1),
M. Montelius
(2),
B. Thorsbro
(3),
H. Jönsson
(4),
G. Mace
(5)
(1)
Lund Observatory
,
Department of Astronomy
,
Theoretical Physics
,
Lund University
,
Box 43
,
SE-221 00 Lund
,
Sweden
,
(2)
Kapteyn Astronomical Institute
,
University of Groningen
,
Landleven 12
,
NL-9747 AD Groningen
,
the Netherlands
,
(3)
Department of Astronomy
,
School of Science
,
The University of Tokyo
,
7-3-1 Hongo
,
Bunkyo-ku
,
Tokyo 113-0033
,
Japan
,
(4)
Materials Science
,
Applied Mathematics
,
Malmö
,
University
,
SE-205 06 Malmö
,
Sweden
,
(5)
Department of Astronomy
,
McDonald Observatory
,
The University of Texas
,
Austin
,
TX 78712
,
USA
http://arxiv.org/abs/2210.04940
Milky Way's eccentric constituents with $Gaia$, APOGEE $&$ GALAH. (arXiv:2206.07744v1 [astro-ph.GA])
Volume 17, Issue 24 - article #13
G. C. Myeong
(1),
Vasily Belokurov
(2, 3),
David S. Aguado
(4, 5),
N. Wyn Evans
(2),
Nelson Caldwell
(1),
James Bradley
(2)
((1) Harvard-Smithsonian Center for Astrophysics,
(2) Institute of Astronomy, Cambridge University,
(3) Center for Computational Astrophysics, Flatiron Institute,
(4) Dipartimento di Fisica e Astrofisica,
(5) INAF/Osservatorio Astrofisico di Arcetri)
http://arxiv.org/abs/2206.07744
The chemical enrichment of the Milky Way disk evaluated using conditional abundances. (arXiv:2206.02772v1 [astro-ph.GA])
Volume 17, Issue 23 - article #4
Bridget Ratcliffe
(1),
Melissa Ness
(2, 3)
((1) Department of Statistics, Columbia University,
(2) Department of Astronomy, Columbia University,
(3) Center for Computational Astrophysics, Flatiron Institute)
http://arxiv.org/abs/2206.02772
Stellar collisions in globular clusters: the origin of multiple stellar populations. (arXiv:2203.02893v1 [astro-ph.GA])
Volume 17, Issue 10 - article #4
Valery Kravtsov
(1),
Sami Dib
(2),
Francisco A. Calderon
(3),
Jose A. Belinchon
(4)
((1) Sternberg Astronomical Institute, Lomonosov Moscow State University, Russia,
(2) Max Planck Institute for Astronomy, Germany,
(3) Departamento de Fisica, Unuversidad Catolica del Norte, Chile,
(4) Departamento de Matematicas, Universidad de Atacama, Chile)
http://arxiv.org/abs/2203.02893
The chemical composition of globular clusters in the Local Group. (arXiv:2112.00081v1 [astro-ph.GA])
Volume 16, Issue 49 - article #10
S. S. Larsen
(1),
P. Eitner
(2,3),
E. Magg
(3),
M. Bergemann
(3,4),
C. A. S. Moltzer
(1),
J. P. Brodie
(5,7),
A. J. Romanowsky
(6,7),
J. Strader
(8)
((1) Department of Astrophysics/IMAPP, Radboud University,
(2) Ruprecht-Karls-Universitaet, Heidelberg,
(3) MPIA, Heidelberg,
(4) Niels Bohr Academy, Niels Bohr Institute, Copenhagen,
(5) Centre for Astrophysics, Supercomputing, Swinburne University,
(6) Department of Physics, Astronomy, San Jose State Univ.,
(7) University of California Observatories, Santa Cruz,
(8) Department of Physics, Astronomy, Michigan State University)
http://arxiv.org/abs/2112.00081
SDSS-IV MaStar: Theoretical Atmospheric Parameters for the MaNGA Stellar Library. (arXiv:2111.05347v1 [astro-ph.GA])
Volume 16, Issue 46 - article #7
Lewis Hill
(1),
Daniel Thomas
(1, 2),
Claudia Maraston
(1),
Renbin Yan
(3),
Justus Neumann
(1),
Andrew Lundgren
(1),
Daniel Lazarz
(3),
Yan-Ping Chen
(4),
Michele Cappellari
(5),
Jon A. Holtzman
(6),
Julie Imig
(6),
Katia Cunha
(7, 8),
Guy Stringfellow
(9),
Dmitry Bizyaev
(10, 11),
David R. Law
(12),
Keivan G. Stassun
(13),
Niv Drory
(14),
Michael Merrifield
(15),
Timothy C. Beers
(16)
((1) Institute of Cosmology, Gravitation, University of Portsmouth, UK,
(2) School of Mathematics, Physics, University of Portsmouth, UK,
(3) Department of Physics, Astronomy, University of Kentucky, USA,
(4) New York University Abu Dhabi, Abu Dhabi, United Arab Emirates,
(5) Department of Physics, University of Oxford, UK,
(6) Department of Astronomy, New Mexico State University, USA,
(7) Observatório Nacional/MCTIC, Brazil,
(8) Steward Observatory, University of Arizona, USA,
(9) Center for Astrophysics, Space Astronomy, University of Colorado, USA,
(10) Apache Point Observatory, New Mexico State University, USA,
(11) Sternberg Astronomical Institute, Moscow State niversity, Russia,
(12) Space Telescope Science Institute, USA,
(13) Vanderbilt University Physics, Astronomy Dept, USA,
(14) McDonald Observatory, The University of Texas at Austin, USA,
(15) School of Physics, Astronomy, University of Nottingham, UK,
(16) Department of Physics, JINA Center for the Evolution of the Elements, University of Notre Dame, USA)
http://arxiv.org/abs/2111.05347
The Influence of 10 Unique Chemical Elements in Shaping the Distribution of Kepler Planets. (arXiv:2111.01753v1 [astro-ph.EP])
Volume 16, Issue 45 - article #9
Robert F. Wilson
(1, 2),
Caleb I. Cañas
(3, 4),
Steven R. Majewski
(1),
Katia Cunha
(5, 6),
Verne V. Smith
(7),
Chad F. Bender
(6),
Suvrath Mahadevan
(3, 4),
Scott W. Fleming
(8),
Johanna Teske
(9),
Luan Ghezzi
(10),
Henrik Jönsson
(11),
Rachael L. Beaton
(12, 13),
Sten Hasselquist
(14),
Keivan Stassun
(15),
Christian Nitschelm
(16),
D. A. García-Hernández
(17, 18),
Christian R. Hayes
(19),
Jamie Tayar
(20, 21)
((1) University of Virginia Department of Astronomy,
(2) NASA Goddard Space Flight Center,
(3) The Pennsylvania State University Department of Astronomy & Astrophysics,
(4) The Pennsylvania State University Center for Exoplanets, Habitable Worlds,
(5) Observatório Nacional,
(6) Steward Observatory,
(7) NSF's NOIRLab,
(8) Space Telescope Science Institute,
(9) Carnegie Earth, Planets Laboratory,
(10) Universidade Federal do Rio de Janeiro,
(11) Malmö University Materials Science, Applied Mathematics,
(12) Princeton University Department of Astrophysical Sciences,
(13) The Observatories of the Carnegie Institution for Science,
(14) University of Utah Department of Physics & Astronomy,
(15) Vanderbilt University Department of Physics, Astronomy,
(16) Universidad de Antofagasta Centro de Astronomía,
(17) Instituto de Astrofísica de Canarias,
(18) Departamento de Astrofísica Universidad de La Laguna,
(19) University of Washington Department of Astronomy,
(20) University of Hawai'i at Manoa Institute for Astronomy,
(21) University of Florida Department of Astronomy)
http://arxiv.org/abs/2111.01753
J-PLUS: Searching for very metal-poor star candidates using the SPEEM pipeline. (arXiv:2109.11600v1 [astro-ph.SR])
Volume 16, Issue 40 - article #2
Carlos Andrés Galarza
(1),
Simone Daflon
(1),
Vinicius M. Placco
(2),
Carlos Allende-Prieto
(3, 4),
Marcelo Borges Fernandes
(1),
Haibo Yuan
(5),
Carlos López-Sanjuan
(6),
Young Sun Lee
(7),
Enrique Solano
(8),
F. Jiménez-Esteban
(8),
David Sobral
(9),
Alvaro Alvarez Candal
(1, 17),
Claudio B. Pereira
(1),
Stavros Akras
(10),
Eduardo Martín
(3, 8),
Yolanda Jiménez Teja
(16),
Javier Cenarro
(6),
David Cristóbal-Hornillos
(6),
Carlos Hernández-Monteagudo
(6),
Antonio Marín-Franch
(6),
Mariano Moles
(6),
Jesús Varela
(6),
Héctor Vázquez Ramió
,
(6),
Jailson Alcaniz
(1),
Renato Dupke
(1, 13, 14, 15),
Alessandro Ederoclite
(11),
Laerte Sodré
,
Jr.
(11),
Raul E. Angulo
(12)
((1) Observatório Nacional - MCTI ON, Rio de Janeiro, Brazil,
(2) NSF's NOIRLab, Tucson, AZ 85719, USA,
(3) Instituto de Astrofísica de Canarias, Tenerife, Spain,
(4) Universidad de La Laguna, Departamento de Astrofísica, Tenerife, Spain,
(5) Department of Astronomy, Beijing Normal University, Beijing, People's Republic of China,
(6) Centro de Estudios de Física del Cosmos de Aragón CEFCA, Unidad Asociada al CSIC, Teruel, Spain,
(7) Department of Astronomy, Space Science, Chungnam National University, South Korea,
(8) Departamento de Astrofísica, Centro de Astrobiología CSIC-INTA, ESAC Campus, Villanueva de la Cañada, Madrid, Spain,
(9) Department of Physics, Lancaster University, Lancaster, UK,
(10) Institute for Astronomy, Astrophysics, Space Applications, Remote Sensing, National Observatory of Athens, GR Penteli, Greece,
(11) Universidade de São Paulo, Instituto de Astronomia, Geofísica e Ciências Atmosféricas, São Paulo, Brazil,
(12) Ikerbasque, Basque Foundation for Science, Bilbao, Spain,
(13) Department of Astronomy, University of Michigan, Ann Arbor, MI USA,
(14) Eureka Scientific Inc., Oakland, CA, USA,
(15) Department of Physics, Astronomy, University of Alabama, Tuscaloosa, AL, USA,
(16) Instituto de Astrofísica de Andalucía-CSIC, Glorieta de la Astronomía, Granada, Spain,
(17) Universidad de Alicante, San Vicente del Raspeig, Alicante, Spain)
http://arxiv.org/abs/2109.11600
Dynamical model of the Milky Way using APOGEE and Gaia data. (arXiv:2106.05286v1 [astro-ph.GA])
Volume 16, Issue 24 - article #2
Maria Selina Nitschai
(1),
Anna-Christina Eilers
(2),
Nadine Neumayer
(1),
Michele Cappellari
(3),
Hans-Walter Rix
(1)
((1) Max Planck Institute for Astronomy,
(2) MIT Kavli Institute for Astrophysics, Space Research,
(3) Sub-department of Astrophysics, Department of Physics, University of Oxford)
http://arxiv.org/abs/2106.05286
On the Use of Field RR Lyrae as Galactic Probes. III. The $alpha$-element abundances. (arXiv:2104.08113v1 [astro-ph.GA])
Volume 16, Issue 17 - article #2
J. Crestani
(1,2,3),
V.F. Braga
(3,4),
M. Fabrizio
(3,4),
G. Bono
(2,3),
C. Sneden
(5),
G.W. Preston
(6),
I. Ferraro
(3),
G. Iannicola
(3),
M. Nonino
(7),
G. Fiorentino
(3),
F. Thévenin
(8),
B. Lemasle
(9),
Z. Prudil
(8),
A. Alves-Brito
(1),
G. Altavilla
(3,4),
B. Chaboyer
(10),
M. Dall'Ora
(11),
V. D'Orazi
(12,13),
C.K. Gilligan
(10),
E. Grebel
(8),
A.J. Koch-Hansen
(9),
H. Lala
(9),
M. Marengo
(14),
S. Marinoni
(3,4),
P.M. Marrese
(3,4),
C.E. Martínez-Vázquez
(15),
N. Matsunaga
(16),
M. Monelli
(17),
J.P. Mullen
(14),
J. Neeley
(18),
R. da Silva
(3,4),
P.B. Stetson
(19),
M. Salaris
(20),
J. Storm
(21),
E. Valenti
(22),
M. Zoccali
(23,24)
((1) Departamento de Astronomia, Universidade Federal do Rio Grande do Sul, Porto Alegre, Brazil,
(2) Dipartimento di Fisica, Università di Roma Tor Vergata, Roma, Italy,
(3) INAF-Osservatorio Astronomico di Roma, Monte Porzio Catone, Italy,
(4) Space Science Data Center, Roma, Italy,
(5) Department of Astronomy, McDonald Observatory, The University of Texas, Austin, TX, USA,
(6) The Observatories of the Carnegie Institution for Science, Pasadena, CA, USA,
(7) INAF-Osservatorio Astronoico di Trieste, Trieste, Italy,
(8) Université de Nice Sophia-antipolis, CNRS, Observatoire de la Côte d'Azur, Laboratoire Lagrange, Nice, France,
(9) Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Heidelberg, Germany,
(10) Department of Physics, Astronomy, Dartmouth College, Hanover, USA,
(11) INAF-Osservatorio Astronomico di Capodimonte, Napoli, Italy,
(12) INAF-Osservatorio Astronomico di Padova, Padova, Italy,
(13) School of Physics, Astronomy, Monash University, Clayton, Melbourne, Australia,
(14) Department of Physics, Astronomy, Iowa State University, Ames, IA, USA,
(15) Cerro Tololo Inter-American Observatory, NSF's National Optical-Infrared Astronomy Research Laboratory, La Serena, Chile,
(16) Department of Astronomy, The University of Tokyo, Tokyo, Japan,
(17) Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain,
(18) Department of Physics, Florida Atlantic University, Boca Raton, FL, USA,
(19) Herzberg Astronomy, Astrophysics, National Research Council, Victoria, BC, Canada,
(20) Astrophysics Research Institute, Liverpool John Moores University, Liverpool, UK,
(21) Leibniz-Institut für Astrophysik Potsdam, Potsdam, Germany,
(22) European Southern Observatory, Garching bei Munchen, Germany,
(23) Instituto Milenio de Astrofísica, Santiago, Chile,
(24) Pontificia Universidad Catolica de Chile, Instituto de Astrofisica, Santiago, Chile)
http://arxiv.org/abs/2104.08113
Metallicity of Galactic RR Lyrae from Optical and Infrared Light Curves: I. Period-Fourier-Metallicity Relations for Fundamental Mode RR Lyrae. (arXiv:2103.09372v1 [astro-ph.SR])
Volume 16, Issue 12 - article #5
Joseph P. Mullen
(1),
Massimo Marengo
(1),
Clara E. Martínez-Vázquez
(2),
Jillian R. Neeley
(3),
Giuseppe Bono
(4, 5),
Massimo Dall'Ora
(6),
Brian Chaboyer
(7),
Frédéric Thévenin
(8),
Vittorio F. Braga
(5, 9),
Juliana Crestani
(4, 5,, 10),
Michele Fabrizio
(5, 9),
Giuliana Fiorentino
(5),
Christina K. Gilligan
(7),
Matteo Monelli
(11, 12),
Peter B. Stetson
(13)
((1) Department of Physics, Astronomy, Iowa State University, Ames, IA, USA,
(2) Cerro Tololo Inter-American Observatory, NSF's National Optical-Infrared Astronomy Research Laboratory, La Serena, Chile,
(3) Department of Physics, Florida Atlantic University, Boca Raton, FL, USA,
(4) Dipartimento di Fisica, Università di Roma Tor Vergata, Roma, Italy,
(5) INAF-Osservatorio Astronomico di Roma, Monte Porzio Catone, Italy,
(6) INAF-Osservatorio Astronomico di Capodimonte, Napoli, Italy,
(7) Department of Physics, Astronomy, Dartmouth College, Hanover, USA,
(8) Université de Nice Sophia-antipolis, CNRS, Observatoire de la Côte d'Azur, Laboratoire Lagrange, Nice, France,
(9) Space Science Data Center, Roma, Italy,
(10) Departamento de Astronomia, Universidade Federal do Rio Grande do Sul, Porto Alegre, Brazil,
(11) Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain,
(12) Departmento de Astrofísica, Universidad de La Laguna, La Laguna, Tenerife, Spain,
(13) Herzberg Astronomy, Astrophysics, National Research Council, Victoria, BC, Canada)
http://arxiv.org/abs/2103.09372
R-process-rich stellar streams in the Milky Way. (arXiv:2102.00066v1 [astro-ph.SR])
Volume 16, Issue 6 - article #5
Maude Gull
(1,2),
Anna Frebel
(2),
Karina Hinojosa
(2),
Ian U. Roederer
(3,4),
Alexander P. Ji
(5),
Kaley Brauer
((1) Department of Astronomy, University of California Berkeley, Berkeley, CA USA,
(2) Department of Physics & Kavli Institute for Astrophysics, Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA,
(3) Department of Astronomy, University of Michigan, Ann Arbor, MI, USA,
(4) Joint Institute for Nuclear Astrophysics - Center for the Evolution of the Elements
(JINA-CEE), USA,
(5) Observatories of the Carnegie Institution for Science, Pasadena, CA, USA)
http://arxiv.org/abs/2102.00066
Estimating distances from parallaxes. V: Geometric and photogeometric distances to 1.47 billion stars in Gaia Early Data Release 3. (arXiv:2012.05220v1 [astro-ph.SR])
Volume 15, Issue 50 - article #4
C. A. L. Bailer-Jones
(1),
J. Rybizki
(1),
M. Fouesneau
(1),
M. Demleitner
(2),
R. Andrae
(1)
((1) Max Planck Institute for Astronomy, Heidelberg,
(2) Astronomisches Rechen-Institut, Heidelberg)
http://arxiv.org/abs/2012.05220
On the Use of Field RR Lyrae as Galactic Probes. II. A new $Delta$S calibration to estimate their metallicity. (arXiv:2012.02284v1 [astro-ph.SR])
Volume 15, Issue 50 - article #6
J. Crestani
(1,2,3),
M. Fabrizio
(3,4),
V.F. Braga
(3,4),
C. Sneden
(5),
G.W. Preston
(6),
I. Ferraro
(3),
G. Iannicola
(3),
G. Bono
(2,3),
A. Alves-Brito
(1),
M. Nonino
(7),
V. D'Orazi
(8,9),
L. Inno
(10),
M. Monelli
(11),
J. Storm
(12),
G. Altavilla
(3,4),
B. Chaboyer
(13),
M. Dall'Ora
(14),
G. Fiorentino
(3),
C.K. Gilligan
(13),
E. Grebel
(15),
H. Lala
(16),
B. Lemasle
(16),
M. Marengo
(17),
S. Marinoni
(3,4),
P.M. Marrese
(3,4),
C.E. Martínez-Vázquez
(18),
N. Matsunaga
(19),
J.P. Mullen
(17),
J. Neeley
(20),
Z. Prudil
(15),
R. da Silva
(3,4),
P.B. Stetson
(21),
F. Thévenin
(15),
E. Valenti
(22),
A.R. Walker
(18),
M. Zoccali
(23,24)
((1) Departamento de Astronomia, Universidade Federal do Rio Grande do Sul, Porto Alegre, Brazil,
(2) Dipartimento di Fisica, Università di Roma Tor Vergata, Roma, Italy,
(3) INAF-Osservatorio Astronomico di Roma, Monte Porzio Catone, Italy,
(4) Space Science Data Center, Roma, Italy,
(5) Department of Astronomy, McDonald Observatory, The University of Texas, Austin, TX, USA,
(6) The Observatories of the Carnegie Institution for Science, Pasadena, CA, USA,
(7) INAF-Osservatorio Astronoico di Trieste, Trieste, Italy,
(8) INAF-Osservatorio Astronomico di Padova, Padova, Italy,
(9) School of Physics, Astronomy, Monash University, Clayton, Melbourne, Australia,
(10) Università degli Studi di Napoli "Parthenope'', Napoli, Italy,
(11) Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain,
(12) Leibniz-Institut für Astrophysik Potsdam, Potsdam, Germany,
(13) Department of Physics, Astronomy, Dartmouth College, Hanover, USA,
(14) INAF-Osservatorio Astronomico di Capodimonte, Napoli, Italy,
(15) Université de Nice Sophia-antipolis, CNRS, Observatoire de la Côte d'Azur, Laboratoire Lagrange, Nice, France,
(16) Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Heidelberg, Germany,
(17) Department of Physics, Astronomy, Iowa State University, Ames, IA, USA,
(18) Cerro Tololo Inter-American Observatory, NSF's National Optical-Infrared Astronomy Research Laboratory, La Serena, Chile,
(19) Department of Astronomy, The University of Tokyo, Tokyo, Japan,
(20) Department of Physics, Florida Atlantic University, Boca Raton, FL, USA,
(21) Herzberg Astronomy, Astrophysics, National Research Council, Victoria, BC, Canada,
(22) European Southern Observatory, Garching bei Munchen, Germany,
(23) Instituto Milenio de Astrofísica, Santiago, Chile,
(24) Pontificia Universidad Catolica de Chile, Instituto de Astrofisica, Santiago, Chile)
http://arxiv.org/abs/2012.02284
The Gaia spectrophotometric standard stars survey -- IV. Results of the absolute photometry campaign. (arXiv:2011.08625v2 [astro-ph.SR] UPDATED)
Volume 15, Issue 48 - article #6
G. Altavilla
(1, 2),
S. Marinoni
(1, 2),
E. Pancino
(3, 2),
S. Galleti
(4),
M. Bellazzini
(4),
N. Sanna
(3),
M. Rainer
(3),
G. Tessicini
(4),
J.M. Carrasco
(5),
A. Bragaglia
(4),
W.J. Schuster
(6),
G. Cocozza
(4),
M. Gebran
(7),
H. Voss
(5),
L. Federici
(4),
E. Masana
(5),
C. Jordi
(5),
M. Monguió
,
(5),
A. Castro
(8, 9),
M.A. Peña-Guerrero
(10),
A. Pérez-Villegas
(11, 6)
((1) INAF -- Osservatorio Astronomico di Roma, Italy,
(2) Space Science Data Center -- ASI, Italy,
(3) INAF -- Osservatorio Astrofisico di Arcetri, Italy,
(4) INAF -- Osservatorio di Astrofisica e Scienza dello Spazio, Italy,
(5) Departament de Física Quàntica i Astrofísica, Institut de Ciències del Cosmos
(ICCUB), Universitat de Barcelona
(IEEC-UB), Spain,
(6) Instituto de Astronomía, Universidad Nacional Autónoma de México, México,
(7) Department of Physics, Astronomy, Notre Dame University-Louaize, Lebanon,
(8) Observatorio Astronómico Nacional, Universidad Nacional Autónoma de México, México,
(9) Consorcio de Investigación del Golfo de México, CICESE, México,
(10) Space Telescope Science Institute, USA,
(11) Universidade de São Paulo, IAG, Brazil)
http://arxiv.org/abs/2011.08625
Low-mass low-metallicity AGB stars as an efficient i-process site explaining CEMP-rs stars. (arXiv:2010.13620v1 [astro-ph.SR])
Volume 15, Issue 44 - article #6
D. Karinkuzhi
(1,2,3),
S. Van Eck
(2),
S. Goriely
(2),
L. Siess
(2),
A. Jorissen
(2),
T. Merle
(2),
A. Escorza
(2,4),
T. Masseron
(5,6)
((1). Department of Physics, Indian Institute of Science, Bangalore, India.560012,
(2). Institut d'Astronomie et d'Astrophysique, Université Libre de Bruxelles, ULB, Campus Plaine C.P. 226, Boulevard du Triomphe, B-1050 Bruxelles, Belgium,
(3). Department of Physics, Jnana Bharathi Campus, Bangalore University, Bangalore, India. 560056,
(4). Institute of Astronomy, KU Leuven, Celestijnenlaan 200D, B-3001 Leuven, Belgium,
(5). Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain,
(6). Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain)
http://arxiv.org/abs/2010.13620
Preliminary Target Selection for the DESI Milky Way Survey (MWS). (arXiv:2010.11284v1 [astro-ph.GA])
Volume 15, Issue 43 - article #4
Carlos Allende Prieto
(1, 2),
Andrew P. Cooper
(3),
Arjun Dey
(4),
Boris T. Gänsicke
(5),
Sergey E. Koposov
(6, 7, 8),
Ting Li
(9, 10),
Christopher Manser
(5),
David L. Nidever
(4, 11),
Constance Rockosi
(12, 13),
Mei-Yu Wang
(7, 14),
David S. Aguado
(8),
Robert Blum
(15),
David Brooks
(16),
Daniel J. Eisenstein
(17),
Yutong Duan
(18),
Sarah Eftekharzadeh
(19),
Enrique Gaztañaga
(20, 21),
Robert Kehoe
(22),
Martin Landriau
(23),
Chien-Hsiu Lee
(4),
Michael E. Levi
(23)
Aaron M. Meisner
(4),
Adam D. Myers
(24),
Joan Najita
(4),
Knut Olsen
(25),
Nathalie Palanque-Delabrouille
(26),
Claire Poppett
(23, 27),
Francisco Prada
(28),
David J. Schlegel
(23),
Michael Schubnell
(29),
Gregory Tarlé
,
(29),
Monica Valluri
(30),
Risa H. Wechsler
(31, 32),
Christophe Yèche
(26)
((1) Instituto de Astrofísica de Canarias,
(2) Universidad de La Laguna,
(3) National Tsing Hua University.
(4) NSF's NOIRLab,
(5) Department of Physics, University of Warwick,
(6) Institute for Astronomy, University of Edinburgh,
(7) McWilliams Center for Cosmology, Carnegie Mellon University,
(8) Institute of Astronomy, University of Cambridge,
(9) Observatories of the Carnegie Institution for Science,
(10) Department of Astrophysical Sciences, Princeton University,
(11) Department of Physics, Montana State University,
(12) Department of Astronomy, Astrophysics, University of California Santa Cruz,
(13) University of California Observatories,
(14) Department of Physics, Carnegie Mellon University,
(15) Vera C. Rubin Observatory/NSF's NOIRLab,
(16) Department of Physics, Astronomy, University College London,
(17) Harvard-Smithsonian Center for Astrophysics,
(18) Physics Department, Boston University,
(19) Department of Physics, Astronomy, The University of Utah,
(20) Institute of Space Sciences
(ICE, CSIC),
(21) Institut d' Estudis Espacials de Catalunya
(IEEC),
(22) Department of Physics, Southern Methodist University,
(23) Lawrence Berkeley National Laboratory,
(24) University of Wyoming,
(25) Community Science, Data Center/NSF's NOIRLab,
(26) IRFU, CEA, Université Paris-Saclay,
(28) Instituto de Astrofisica de Andalucía,
(29) Department of Physics, University of Michigan,
(30) Department of Astronomy, University of Michigan,
(31) Kavli Institute for Particle Astrophysics, Cosmology, Department of Physics,
(32) SLAC National Accelerator Laboratory)
http://arxiv.org/abs/2010.11284
The stochastic enrichment of Population II stars. (arXiv:2010.10532v1 [astro-ph.GA])
Volume 15, Issue 43 - article #6
Louise Welsh
(1),
Ryan Cooke
(1),
Michele Fumagalli
(2,1)
((1) Centre for Extragalactic Astronomy, Durham University,
(2) Physics department, University of Milano Bicocca)
http://arxiv.org/abs/2010.10532
An extremely metal-deficient globular cluster in the Andromeda Galaxy. (arXiv:2010.07395v1 [astro-ph.GA])
Volume 15, Issue 42 - article #1
S. S. Larsen
(1),
A. J. Romanowsky
(2,4),
J. P. Brodie
(3,4),
A. Wasserman
(4)
((1) Department of Astrophysics/IMAPP, Radboud University, Nijmegen, The Netherlands,
(2) Department of Physics, Astronomy, San Jose State University, San Jose, CA, USA,
(3) Centre for Astrophysics, Supercomputing, Swinburne University of Technology, Hawthorn, VIC, Australia,
(4) University of California Observatories, University of California, Santa Cruz, CA, USA)
http://arxiv.org/abs/2010.07395
Constraining Nucleosynthesis in Two CEMP Progenitors Using Fluorine. (arXiv:2008.10136v1 [astro-ph.SR])
Volume 15, Issue 35 - article #2
A. A. Mura-Guzmán
(1,2),
D. Yong
(1,2),
C. Abate
(3),
A. Karakas
(4,2),
C. Kobayashi
(5,2),
H. Oh
(6),
S. Chun
(6),
G. Mace
(7).
((1) Research School of Astronomy, Astrophysics, Australian National University, Australia,
(2) ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions
(ASTRO 3D), Australia,
(3) Deep Blue Srl, Rome, Italy,
(4) School of Physics, Astronomy, Monash University, Australia,
(5) Centre for Astrophysics Research, University of Hertfordshire, UK,
(6) Korea Astronomy, Space Science Institute, Republic of Korea,
(7) Department of Astronomy, McDonald Observatory, University of Texas at Austin, USA.)
http://arxiv.org/abs/2008.10136
Mapping the Galactic disk with the LAMOST and $Gaia$ Red clump sample: V: On the origin of the "young" [$alpha$/Fe]-enhanced stars. (arXiv:2008.10218v1 [astro-ph.GA])
Volume 15, Issue 35 - article #5
Weixiang Sun
(1),
Yang Huang
(1),
Haifeng Wang
(1),
Chun Wang
(2,3),
Meng Zhang
(2,3),
Xinyi Li
(1),
Bingqiu Chen
(1),
Huawei Zhang
(2,3),
Dandan Wei
(4),
Dengkai Jiang
(4),
Xiaowei Liu
(1),
((1) South-Western Institute for Astronomy Research, Yunnan University,
(2) Department of Astronomy, Peking University,
(3) Kavli Institute for Astronomy, Astrophysics, Peking University,
(4) Yunnan Observatories, Chinese Academy of Sciences)
http://arxiv.org/abs/2008.10218
SkyMapper Southern Survey: Second Data Release (DR2). (arXiv:2008.10359v1 [astro-ph.IM])
Volume 15, Issue 35 - article #6
Christopher A. Onken
(1),
Christian Wolf
(1),
Michael S. Bessell
(1),
Seo-Won Chang
(1),
Gary S. Da Costa
(1),
Lance C. Luvaul
(1),
Dougal Mackey
(1),
Brian P. Schmidt
(1),
Li Shao
(1, 2)
((1) Research School of Astronomy & Astrophysics, Australian National University,
(2) Kavli Institute for Astronomy, Astrophysics, Peking University)
http://arxiv.org/abs/2008.10359
The Gaia-ESO Survey: Membership probabilities for stars in 32 open clusters from 3D kinematics. (arXiv:2006.09423v1 [astro-ph.SR])
Volume 15, Issue 25 - article #13
R. J. Jackson
(1)
R. D. Jeffries
(1),
N. J. Wright
(1),
S. Randich
(2),
G. Sacco
(2),
E. Pancino
(2),
T. Cantat-Gaudin
(3),
G. Gilmore
(4),
A. Vallenari
(5),
T. Bensby
(6),
A. Bayo
(7),
M. T. Costado
(8),
E. Franciosini
(2),
A. Gonneau
(4),
A. Hourihane
(4),
J. Lewis
(4),
L. Monaco
(9),
L. Morbidelli
(2),
C. Worley
(4)
((1) Keele University,
(2) Osservatorio Astrofisco di Arcetri,
(3) Institut de Ciencies del Cosmos, Barcelona,
(4) Institute of Astronomy, Cambridge,
(5) Osservatorio Astronomico di Padova,
(6) Lund Observatory,
(7) Instituto de Fisica y Astronomia, Valparaiso,
(8) Departamento de Didactica, Cadiz,
(9) Departamento de Ciencias Fisicas, Santiago)
http://arxiv.org/abs/2006.09423
Wide binaries are rare in open clusters. (arXiv:2006.06679v1 [astro-ph.SR])
Volume 15, Issue 25 - article #16
N.R. Deacon
(1),
A.L. Kraus
(2).
((1) Max Planck Institute for Astronomy,
(2) Department of Astronomy, The University of Texas at Austin)
http://arxiv.org/abs/2006.06679
Elemental Abundances in M31: Iron and Alpha Element Abundances in M31's Outer Halo
Volume 15, Issue 24 - article #6
Karoline M. Gilbert
(1, 2),
Jennifer Wojno
(2),
Evan N. Kirby
(3),
Ivanna Escala
(3, 4),
Rachael L. Beaton
(4, 5, 6, 7),
Puragra Guhathakurta
(8),
Steven R. Majewski
(9)
((1) Space Telescope Science Institute,
(2) Department of Physics & Astronomy, Johns Hopkins University,
(3) California Institute of Technology,
(4) Department of Astrophysical Sciences, Princeton University,
(5) The Observatories of the Carnegie Institution for Science,
(6) Hubble Fellow,
(7) Carnegie-Princeton Fellow,
(8) UCO/Lick Observatory, Department of Astronomy & Astrophysics, University of California Santa Cruz,
(9) Department of Astronomy, University of Virginia)
http://arxiv.org/abs/2006.05430
High-precision abundances of elements in solar-type stars. Evidence of two distinct sequences in abundance-age relations. (arXiv:2006.06013v1 [astro-ph.SR])
Volume 15, Issue 24 - article #9
P. E. Nissen
,
J. Christensen-Dalsgaard
,
J. R. Mosumgaard
,
V. Silva Aguirre
,
E. Spitoni
,
K. Verma.
(Stellar Astrophysics Centre, Department of Physics, Astronomy, Aarhus University, Denmark.)
http://arxiv.org/abs/2006.06013
Hydrodynamics of core-collapse supernovae and their progenitors
Volume 15, Issue 24 - article #10
B. Müller
(Monash University, School of Physics and Astronomy)
http://arxiv.org/abs/2006.05083
Chronologically dating the early assembly of the Milky Way. (arXiv:2006.01783v1 [astro-ph.GA])
Volume 15, Issue 23 - article #4
Josefina Montalbán
(1),
John Ted Mackereth
(1),
Andrea Miglio
(1, 2),
Fiorenzo Vincenzo
(3,4, 1),
Cristina Chiappini
(5),
Gaël Buldgen
(6),
Benoît Mosser
(7),
Arlette Noels
(8),
Richard Scuflaire
(8),
Mathieu Vrard
(4, 10),
Emma Willett
(1, 2),
Guy R. Davies
(1, 2),
Oliver Hall
(1, 2)
Martin Bo Nielsen
(1,2, 11),
Saniya Khan
(1, 2),
Ben M. Rendle
(1, 2),
Walter E. van Rossem
(1, 2),
Jason W. Ferguson
(9),
William J. Chaplin
(1, 2)
((1) School of Physics, Astronomy, University of Birmingham, UK,
(2) SAC, Aarhus University, Denmark,
(3) Center for Cosmology, AstroParticle Physics, The Ohio State University, USA,
(4) Departement of Astronomy, The Ohio State University, USA,
(5) Leibniz-Institut fur Astrophysik Potsdam, Germany,
(6) Observatoire de Genève, Université de Genève, Switzerland,
(7) LESIA, Observatoire de Paris, Université de Paris, France,
(8) STAR Institute, University of Liège, Belgium,
(9) Departement of Physics, Wichita State University, USA,
(10) Instituto de Astrofśica e Ciências do Espaço, Universidade do Porto, Portugal,
(11) Center for Space Science, NYUAD, New York University Abu Dhabi, United Arab Emirates)
http://arxiv.org/abs/2006.01783
Production of Lithium in Primordial Supernovae. (arXiv:2002.04749v1 [astro-ph.SR])
Volume 15, Issue 7 - article #7
Alexander Heger
(1),
Stan Woosley
(2)
((1) School of Physics, Astronomy, Monash University, Australia,
(2) Department of Astronomy, Astrophysics, University of California at Santa Cruz, USA)
http://arxiv.org/abs/2002.04749
Identification of strontium in the merger of two neutron stars. (arXiv:1910.10510v1 [astro-ph.HE])
Volume 14, Issue 43 - article #4
Darach Watson
(1, 2),
Camilla J. Hansen
(3),
Jonatan Selsing
(1, 2),
Andreas Koch
(4),
Daniele B. Malesani
(1, 2, 5),
Anja C. Andersen
(1),
Johan P. U. Fynbo
(1, 2),
Almudena Arcones
(6, 7),
Andreas Bauswein
(7, 8),
Stefano Covino
(9),
Aniello Grado
(10),
Kasper E. Heintz
(1, 2, 11),
Leslie Hunt
(12),
Chryssa Kouveliotou
(13, 14),
Giorgos Leloudas
(1, 5),
Andrew Levan
(15, 16),
Paolo Mazzali
(17, 18),
Elena Pian
(19)
((1) Niels Bohr Institute, University of Copenhagen,
(2) Cosmic Dawn Center
(DAWN),
(3) Max-Planck-Institut für Astronomie, Heidelberg,
(4) Zentrum für Astronomie der Universität Heidelberg,
(5) DTU Space, Technical University of Denmark,
(6) Institut für Kernphysik, Technische Universität Darmstadt,
(7) GSI Helmholtzzentrum für Schwerionenforschung GmbH, Darmstadt,
(8) Heidelberger Institut für Theoretische Studien, Heidelberg,
(9) INAF / Brera Astronomical Observatory, Merate,
(10) INAF-OACN, Naples,
(11) Centre for Astrophysics, Cosmology, University of Iceland,
(12) INAF - Osservatorio Astrofisico di Arcetri, Firenze,
(13) Physics Department, the George Washington University,
(14) Astronomy, Physics, Statistics Institute of Sciences
(APSIS), Washington, DC,
(15) Department of Astrophysics/IMAPP, Radboud University Nijmegen,
(16) Department of Physics, University of Warwick,
(17) Astrophysics Research Institute, Liverpool John Moores University,
(18) Max-Planck Institute for Astrophysics, Garching,
(19) INAF, Astrophysics, Space Science Observatory, Bologna)
http://arxiv.org/abs/1910.10510
Modelling the chemical enrichment of Population III supernovae: The origin of the metals in near-pristine gas clouds. (arXiv:1906.00009v2 [astro-ph.SR] UPDATED)
Volume 14, Issue 33 - article #4
Louise Welsh
(1),
Ryan Cooke
(1),
Michele Fumagalli
(1,2)
((1) Centre for Extragalactic Astronomy, Durham University,
(2) Institute for Computational Cosmology, Durham University)
http://arxiv.org/abs/1906.00009
Evidence for Sub-Chandrasekhar Type Ia Supernovae from Stellar Abundances in Dwarf Galaxies. (arXiv:1906.10126v1 [astro-ph.SR])
Volume 14, Issue 26 - article #4
Evan N. Kirby
(1),
Justin L. Xie
(2),
Rachel Guo
(2),
Mithi A. C. de los Reyes
(1),
Maria Bergemann
(3),
Mikhail Kovalev
,
(3),
Ken J. Shen
(4),
Anthony L. Piro
(5),
Andrew McWilliam
(5)
((1) Caltech,
(2) Harvard College,
(3) Max-Planck Institute for Astronomy,
(4) UC Berkeley,
(5) Carnegie Observatories)
http://arxiv.org/abs/1906.10126
Formation of Second Generation Stars in Globular Clusters. (arXiv:1906.09137v1 [astro-ph.SR])
Volume 14, Issue 26 - article #5
F. Calura
(1),
A. D'Ercole
(1),
E. Vesperini
(2),
E. Vanzella
(1),
A. Sollima
(1)
((1) INAF-OAS, Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Italy,
(2) Department of Astronomy, Indiana University, Bloomington, USA)
http://arxiv.org/abs/1906.09137
Chemical Compositions of Field and Globular Cluster RR~Lyrae Stars: II. omega Centauri. (arXiv:1906.08550v1 [astro-ph.SR])
Volume 14, Issue 25 - article #2
D. Magurno
(1, 2, 3),
C. Sneden
(4),
G. Bono
(1, 2),
V. F. Braga
(5, 6),
M. Mateo
(7),
S. E. Persson
(8),
G. Preston
(8),
F. Thevenin
(9),
R. da Silva
(10),
M. Dall'Ora
(11),
M. Fabrizio
(2, 10),
I. Ferraro
(2),
G. Fiorentino
(12),
G. Iannicola
(2),
L. Inno
(13),
M. Marengo
(14),
S. Marinoni
(10),
P. M. Marrese
(10),
C. E. Martinez-Vazquez
(15),
N. Matsunaga
(16),
M. Monelli
(17),
J. R. Neeley
(18),
M. Nonino
(19),
A. R. Walker
(15)
((1) University of Roma Tor Vergata - Department of Physics - Roma - Italy,
(2) INAF Osservatorio Astronomico di Roma - Monte Porzio Catone RM - Italy,
(3) University of Bologna - Department of Physics, Astronomy - Bologna - Italy,
(4) Department of Astronomy, McDonald Observatory - The University of Texas - Austin - TX - USA,
(5) Instituto Milenio de Astrofisica - Santiago - Chile,
(6) Departamento de Fisica - Facultad de Ciencias Exactas - Universidad Andres Bello - Las Condes - Santiago - Chile,
(7) Department of Astronomy - University of Michigan - Ann Arbor - MI - USA,
(8) Observatories of the Carnegie Institution for Science - Pasadena - CA 91101 - USA,
(9) Universite de La Cote d'Azur - OCA - Laboratoire Lagrange CNRS - Nice Cedex - France,
(10) SSDC - via del Politecnico snc - I-00133 Roma - Italy,
(11) INAF Osservatorio Astronomico di Capodimonte - Salita Moiariello 16 - Napoli - Italy,
(12) INAF Osservatorio Astronomico di Bologna - Via Ranzani 1 - Bologna - Italy,
(13) Max Planck Institute fur Astronomie - Konigstuhl - Heidelberg - Germany,
(14) Department of Physics, Astronomy - Iowa State University - Zaffarano - Ames - IA - USA,
(15) Cerro Tololo Inter-American Observatory - National Optical Astronomy Observatory - Casilla - La Serena - Chile,
(16) Department of Astronomy - The University of Tokyo - Hongo - Bunkyo-ku - Tokyo - Japan,
(17) IAC - Instituto de Astrofsica de Canarias - Calle Via Lactea - La Laguna - Tenerife - Espana,
(18) Department of Physics - Florida Atlantic University - Boca Raton - FL - USA,
(19) INAF Osservatorio Astronomico di Trieste - Trieste - Italy)
http://arxiv.org/abs/1906.08550
The Age and Metallicity Dependence of the Near-Infrared Magnitudes of Red Clump Stars. (arXiv:1904.12874v1 [astro-ph.SR])
Volume 14, Issue 18 - article #3
Hiroki Onozato
(1, 2),
Yoshifusa Ita
(1),
Yoshikazu Nakada
(3),
Shogo Nishiyama
(4)
((1) Astronomical Institute, Graduate School of Science, Tohoku University, Aramaki Aoba, Aoba-ku, Sendai, Miyagi, Japan,
(2) Nishi-Harima Astronomical Observatory, Center for Astronomy, Institute of Natural, Environmental Sciences, University of Hyogo, Nishigaichi, Sayo-cho, Sayo-gun, Hyogo, Japan,
(3) Kiso Observatory, Institute of Astronomy, School of Science, The University of Tokyo, Mitake, Kiso-machi, Kiso-gun, Nagano, Japan,
(4) Miyagi University of Education, Aramaki Aoba, Aoba-ku, Sendai, Miyagi, Japan)
http://arxiv.org/abs/1904.12874
HST resolves stars in a tiny body falling on the dwarf galaxy DDO 68. (arXiv:1904.01986v1 [astro-ph.GA])
Volume 14, Issue 14 - article #6
F. Annibali
(1),
M. Bellazzini
(1),
M. Correnti
(2),
E. Sacchi
(2),
M. Tosi
(1),
M. Cignoni
(3),
A. Aloisi
(2),
D. Calzetti
(4),
L. Ciotti
(5),
F. Cusano
(1),
J. Lee
(6),
C. Nipoti
(5)
((1) INAF-Astrophysics, Space Science Observatory, Bologna, Italy
(2) Space Telescope Science Institute, Baltimore, USA
(3) Dipartimento di Fisica, Universita' di Pisa, Italy
(4) Department of Astronomy, University of Massachusetts-Amherst, USA
(5) Dipartimento di Fisica e Astronomia, Universita' di Bologna, Italy
(6) Caltech-IPAC, USA)
http://arxiv.org/abs/1904.01986
The Fornax 3D project: Thick disks in a cluster environment. (arXiv:1904.01260v1 [astro-ph.GA])
Volume 14, Issue 14 - article #11
F. Pinna
(1, 2),
J. Falcón-Barroso
(1, 2),
M. Martig
(3),
L. Coccato
(4),
E. M. Corsini
(5, 6),
P.T. de Zeeuw
(7, 8),
D.A. Gadotti
(4),
E. Iodice
(9),
R. Leaman
(10),
M. Lyubenova
(4),
I. Martín-Navarro
(11, 10),
L. Morelli
(12, 6),
M. Sarzi
(13),
G. van de Ven
(14, 4),
S. Viaene
(15, 16),
R.M. McDermid
(17, 18)
((1) Instituto de Astrofísica de Canarias,
(2) Depto. Astrofísica, Universidad de La Laguna,
(3) Astrophysics Research Institute, Liverpool John Moores University,
(4) European Southern Observatory,
(5) Dipartimento di Fisica e Astronomia 'G. Galilei', Università di Padova,
(6) INAF-Osservatorio Astronomico di Padova,
(7) Sterrewacht Leiden, Leiden University,
(8) Max-Planck-Institut fuer extraterrestrische Physik,
(9) INAF-Osservatorio Astronomico di Capodimonte,
(10) Max-Planck Institut fuer Astronomie,
(11) University of California Observatories,
(12) Instituto de Astronomía y Ciencias Planetarias, Universidad de Atacama,
(13) Armagh Observatory, Planetarium,
(14) Department of Astrophysics, University of Vienna,
(15) Sterrenkundig Observatorium, Universiteit Gent,
(16) Centre for Astrophysics Research, University of Hertfordshire,
(17) Department of Physics, Astronomy, Macquarie University,
(18) Australian Astronomical Observatory)
http://arxiv.org/abs/1904.01260
The fourth data release of the Kilo-Degree Survey: ugri imaging and nine-band optical-IR photometry over 1000 square degrees. (arXiv:1902.11265v1 [astro-ph.GA])
Volume 14, Issue 9 - article #7
K. Kuijken
(1),
C. Heymans
(2),
A. Dvornik
(1),
H. Hildebrandt
(3,4),
J.T.A. de Jong
(5),
A.H. Wright
(4),
T. Erben
(4),
M. Bilicki
(1,6),
B. Giblin
(2),
H.-Y. Shan
(4,7),
F. Getman
(8),
A. Grado
(8),
H. Hoekstra
(1),
L. Miller
(9),
N. Napolitano
(10,8),
M. Paolilo
(11),
M. Radovich
(12),
P. Schneider
(4),
W. Sutherland
(13),
M. Tewes
(4),
C. Tortora
(14),
E.A. Valentijn
(5),
G.A. Verdoes Kleijn
(5)
((1) Leiden Observatory,
(2) SUPA, Edinburgh,
(3) Astronomisches Inst., Bochum,
(4) Argelander Inst., Bonn,
(5) Kapteyn Astronomical Inst., Groningen,
(6) Ctr. For Theoretical Physics, Polish Academy of Sciences, Warsaw,
(7) Shanghai Astronomical Observatory,
(8) INAF Capodimonte,
(9) Dept. of Physics, Oxford,
(10) School of Physics, Astronomy, Sun Yat-sen University, Guangzhou,
(11) Dept. of Physics, Univ. Federico II, Naples,
(12) INAF Padua,
(13) School of Physics, Astronomy, Queen Mary University, London,
(14) INAF Arcetri)
http://arxiv.org/abs/1902.11265
Mapping the stellar age of the Milky Way bulge with the VVV. I. The method. (arXiv:1902.01695v1 [astro-ph.GA])
Volume 14, Issue 6 - article #2
F. Surot
(1, 4),
E. Valenti
(1),
S. L. Hidalgo
(2, 3),
M. Zoccali
(4, 5),
E. Sökmen
(2, 3),
M. Rejkuba
(1, 6),
D. Minniti
(5, 7, 8),
O. A. Gonzalez
(9),
S. Cassisi
(10, 11),
A. Renzini
(12),
A. Weiss
(13)
((1) European Southern Observatory,
(2) Instituto de Astrofísica de Canarias,
(3) Department of Astrophysics University of La Laguna,
(4) Instituto de Astrofísica Pontificia Universidad Católica de Chile,
(5) Millennium Institute of Astrophysics,
(6) Excellence Cluster Universe,
(7) Departamento de Ciencias Físicas Universidad Andrés Bello,
(8) Vatican Observatory,
(9) Institute for Astronomy University of Edinburgh,
(10) INAF - Astronomical Observatory of Abruzzo,
(11) INFN,
(12) INAF - Osservatorio Astronomico di Padova,
(13) Max-Planck-Institut für Astrophysik)
http://arxiv.org/abs/1902.01695
On a new method to estimate distance, reddening and metallicity of RR Lyrae stars using optical/near-infrared ($B$,$V$,$I$,$J$,$H$,$K$) mean magnitudes: $omega$ Centauri as a first test case. (arXiv:1811.07069v1 [astro-ph.SR])
Volume 13, Issue 47 - article #2
G. Bono
(1, 2),
G. Iannicola
(2),
V.F. Braga
(3, 4),
I. Ferraro
(2),
P.B. Stetson
(5),
D. Magurno
(1),
N. Matsunaga
(6),
R.L. Beaton
(7),
R. Buonanno
(8),
B. Chaboyer
(9),
M. Dall'Ora
(10),
M. Fabrizio
(2, 11),
G. Fiorentino
(12),
W.L. Freedman
(13,7),
C.K. Gilligan
(9),
B.F. Madore
(7),
M. Marconi
(10),
M. Marengo
(14),
S. Marinoni
(2, 11),
P. Marrese
(2, 11),
C.E. Martinez-Vazquez
(15),
M. Mateo
(16),
M. Monelli
(17, 18),
J.R. Neeley
(19),
M. Nonino
(20),
C. Sneden
(21),
F. Thevenin
(22),
E. Valenti
(23),
A.R. Walker
(15)
((1) Department of Physics, Università di Roma Tor Vergata, Roma, Italy,
(2) INAF-Osservatorio Astronomico di Roma, Monte Porzio Catone, Italy,
(3) Instituto Milenio de Astrofisica, Santiago, Chile,
(4) Departamento de Fisica, Facultad de Ciencias Exactas, Universidad Andres Bello, Santiago, Chile,
(5) NRC-Herzberg, Dominion Astrophysical Observatory, Victoria BC, Canada,
(6) Kiso Observatory, Institute of Astronomy, School of Science, The University of Tokyo, Nagano Japan,
(7) The Observatories of the Carnegie Institution for Science, Pasadena, CA, USA,
(8) INAF-Osservatorio Astronomico d'Abruzzo, Teramo, Italy,
(9) Department of Physics, Astronomy, Dartmouth College, Hanover, NH, USA,
(10) INAF-Osservatorio Astronomico di Capodimonte, Napoli, Italy,
(11) SSDC, Roma, Italy,
(12) INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Bologna, Italy,
(13) Department of Astronomy, Astrophysics, University of Chicago, Chicago, IL, USA,
(14) Department of Physics, Astronomy, Iowa State University, Ames, IA, USA,
(15) Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, La Serena, Chile,
(16) Department of Astronomy, University of Michigan, Ann Arbor, MI, USA,
(17) Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain,
(18) Departamento de Astrofisica, Universidad de La Laguna, Tenerife, Spain,
(19) Department of Physics, Florida Atlantic University, Boca Raton, FL 33431, USA,
(20) INAF-Osservatorio Astronomico di Trieste, Trieste, Italy,
(21) Department of Astronomy, McDonald Observatory, The University of Texas, Austin, TX, USA,
(22) Universite de Nice Sophia-antipolis, CNRS, Observatoire de la Cote d'Azur, Laboratoire Lagrange, Nice, France,
(23) European Southern Observatory, Garching bei Munchen, Germany)
http://arxiv.org/abs/1811.07069
Local disc model in view of Gaia DR1 and RAVE data. (arXiv:1810.00814v1 [astro-ph.GA])
Volume 13, Issue 40 - article #5
K. Sysoliatina
(1),
A. Just
(1),
I. Koutsouridou
(2),
E.K. Grebel
(1),
G. Kordopatis
(8),
M. Steinmetz
(10),
O. Bienaymé
,
(9),
B.K. Gibson
(3),
J. Navarro
(7),
W. Reid
(5,6),
G. Seabroke
(4)
((1) Astronomisches Rechen-Institut, Heidelberg, Germany,
(2) Observatoire de Paris, France,
(3) E.A. Milne Centre for Astrophysics, University of Hull, UK,
(4) Mullard Space Science Laboratory, University College London, UK,
(5) Department of Physics, Astronomy, Macquarie University, Sydney, Australia,
(6) Western Sydney University, Australia,
(7) Senior CIfAR Fellow, University of Victoria, Canada,
(8) Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, France,
(9) Observatoire astronomique de Strasbourg, Université de Strasbourg, France,
(10) Leibniz Institut für Astrophysik Potsdam, Germany)
http://arxiv.org/abs/1810.00814
The faint end of the Centaurus A satellite luminosity function. (arXiv:1809.05103v1 [astro-ph.GA])
Volume 13, Issue 38 - article #9
D. Crnojević
,
(1,2),
D. J. Sand
(3),
P. N. Bennet
(2),
S. Pasetto
(4,1),
K. Spekkens
(5),
N. Caldwell
(6),
P. Guhathakurta
(7),
B. McLeod
(6),
A. Seth
(8),
J. D. Simon
(4),
J. Strader
(9),
E. Toloba
(10)
((1) University of Tampa, Tampa, FL, USA,
(2) Department of Physics & Astronomy, Texas Tech University, Lubbock, TX, USA,
(3) Department of Astronomy, Steward Observatory, University of Arizona, Tucson, AZ, USA,
(4) Observatories of the Carnegie Institution for Science, Pasadena, CA, USA,
(5) Department of Physics & Space Science, Royal Military College of Canada, Kingston, Ontario, Canada,
(6) Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA,
(7) Department of Astronomy & Astrophysics, University of California Santa Cruz, CA, USA,
(8) Department of Physics, Astronomy, University of Utah, Salt Lake City, UT, USA,
(9) Department of Physics, Astronomy, Michigan State University, East Lansing, MI, USA,
(10), Department of Physics, University of the Pacific, Stockton, CA, USA)
http://arxiv.org/abs/1809.05103
Structure and kinematics of Type II Cepheids in the Galactic bulge based on near-infrared VVV data. (arXiv:1808.10838v1 [astro-ph.GA])
Volume 13, Issue 36 - article #9
V.F. Braga
(1,2),
A. Bhardwaj
(3),
R. Contreras Ramos
(1,4),
D. Minniti
(1,2,5),
G. Bono
(6,7),
R. de Grijs
(8,9),
J.H. Minniti
(4,10),
M. Rejkuba
(11)
((1) Instituto Milenio de Astrofísica, Santiago, Chile,
(2) Departamento de Física, Facultad de Ciencias Exactas, Universidad Andrés Bello, Santiago, Chile,
(3) Kavli Institute for Astronomy, Astrophysics, Peking University, China,
(4) Pontificia Universidad Católica de Chile, Instituto de Astrofísica, Macul, Chile,
(5) Vatican Observatory, Italy,
(6) Department of Physics, Università di Roma Tor Vergata, Italy,
(7) INAF-Osservatorio Astronomico di Roma, Italy,
(8) Department of Physics, Astronomy, Macquarie University, Balaclava Road, Sydney, Australia,
(9) International Space Science Institute--Beijing, Zhongguancun, China,
(10) European Southern Observatory, Santiago, Chile,
(11) European Southern Observatory, Garching, Germany)
http://arxiv.org/abs/1808.10838
The GeMS/GSAOI Galactic Globular Cluster Survey (G4CS) I: A Pilot Study of the stellar populations in NGC 2298 and NGC 3201. (arXiv:1808.05271v1 [astro-ph.GA])
Volume 13, Issue 34 - article #4
Stephanie Monty
(1,2),
Thomas H. Puzia
(3),
Bryan W. Miller
(4),
Eleazar R. Carrasco
(4),
Mirko Simunovic
(5),
Mischa Schirmer
(4,6),
Peter B. Stetson
(7),
Santi Cassisi
(8),
Kim A. Venn
(1),
Aaron Dotter
(9),
Paul Goudfrooij
(10),
Sibilla Perina
(11),
Peter Pessev
(12),
Ata Sarajedini
(13),
Matthew A. Taylor
(5)
((1) Department of Physics, Astronomy, University of Victoria, Canada,
(2) Research School of Astronomy, Astrophysics, Australian National University, Australia,
(3) Institute of Astrophysics, Pontificia Universidad Catolica de Chile, Santiago, Chile,
(4) Gemini Observatory/AURA, Southern Operations Center, Chile,
(5) Gemini Observatory, USA,
(6) Max-Planck-Institut fuer Astronomie, Germany,
(7) Herzberg Astronomy, Astrophysics, National Research Council Canada, Canada,
(8) INAF - Astronomical Observatory of Abruzzo, Italy,
(9) Harvard-Smithsonian Center for Astrophysics, USA,
(10) Space Telescope Science Institute, USA,
(11) INAF - Astronomical Observatory of Torino, Italy,
(12) Gran Telescopio Canarias, Instituto de Astrofisica de Canarias, Universidad de La Laguna, Spain,
(13) Department of Astronomy, University of Florida, 211 Bryant Space Science Center Gainesville, FL, USA)
http://arxiv.org/abs/1808.05271
When binaries keep track of recent nucleosynthesis: The Zr - Nb pair in extrinsic stars as an s-process diagnostic. (arXiv:1807.06332v1 [astro-ph.SR])
Volume 13, Issue 29 - article #16
D. Karinkuzhi
(1),
S. Van Eck
(1),
A. Jorissen
(1),
S. Goriely
(1),
L. Siess
(1),
T. Merle
(1),
A. Escorza
(1, 2),
M. Van der Swaelmen
(1),
H.M.J. Boffin
(3),
T. Masseron
(4,5),
S. Shetye
(1,2),
B. Plez
(6)
((1). Institute of Astronomy, Astrophysics, University of Brussels, ULB, Campus Plaine C.P. 226, Boulevard du Triomphe, B-1050 Bruxelles, Belgium.
(2) Institute of Astronomy, KU Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium.
(3) ESO, Karl Schwarzschild Strasse 2, D-85748 Garching bei Munchen, Germany.
(4) Instituto de Astrofisica de Canarias, E-38205 La Laguna, Tenerife, Spain.
(5) Departamento de Astrofisica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain.
(6) Laboratoire Univers et Particules de Montpellier, Universite Montpellier, CNRS, 34095, Montpellier Cedex 05, France.)
http://arxiv.org/abs/1807.06332
$Lambda$CDM Cosmology for Astronomers. (arXiv:1804.10047v1 [astro-ph.CO])
Volume 13, Issue 17 - article #1
J. J. Condon
(1),
A. M. Matthews
(2)
((1) National Radio Astronomy Observatory,
(2) University of Virginia)
http://arxiv.org/abs/1804.10047
Gaia Data Release 2. Summary of the contents and survey properties. (arXiv:1804.09365v1 [astro-ph.GA])
Volume 13, Issue 17 - article #9
Gaia Collaboration: A.G.A. Brown
(1),
A. Vallenari
(2),
T. Prusti
(3),
J.H.J. de Bruijne
(3),
C. Babusiaux
(4,5),
C.A.L. Bailer-Jones
(6)
((1) Leiden Observatory, Leiden University,
(2) INAF - Osservatorio astronomico di Padova,
(3) ESA/ESTEC,
(4) GEPI, Observatoire de Paris,
(5) Univ. Grenoble Alpes,
(6) Max Planck Institute for Astronomy)
http://arxiv.org/abs/1804.09365
The local rotation curve of the Milky Way based on SEGUE and RAVE data. (arXiv:1802.07658v1 [astro-ph.GA])
Volume 13, Issue 8 - article #12
K. Sysoliatina
(1),
A. Just
(1),
O. Golubov
(2,3,4),
Q.A. Parker
(5,6),
E.K. Grebel
(1),
G. Kordopatis
(17),
T. Zwitter
(15),
J. Bland-Hawthorn
(14),
B.K. Gibson
(8),
A. Kunder
(16),
U. Munari
(7),
J. Navarro
(12),
W. Reid
(10,11),
G. Seabroke
(9),
M.Steinmetz
(18),
F. Watson
(13)
((1) Astronomisches Rechen-Institut, Heidelberg, Germany,
(2) Schools of Physics, Technology, Karazin Kharkiv National University, Kharkiv, Ukraine,
(3) Institute of Astronomy, Karazin Kharkiv National University, Kharkiv, Ukraine,
(4) Department of Aerospace Engineering Sciences, University of Colorado at Boulder, USA,
(5) Department of Physics, the University of Hong Kong, China,
(6) The Laboratory for Space Research, the university of Hong Kong, China,
(7) INAF Astronomical Observatory of Padova, Italy,
(8) E.A. Milne Centre for Astrophysics, University of Hull, UK,
(9) Mullard Space Science Laboratory, University College London, UK,
(10) Department of Physics, Astronomy, Macquarie University, Sydney, Australia,
(11) Western Sydney University, Australia,
(12) Senior CIfAR Fellow, University of Victoria, Canada,
(13) Australian Astronomical Observatory
(14) Sydney Institute for Astronomy, School of Physics, University of Sydney, Australia,
(15) Faculty of Mathematics, Physics, University of Ljubljana, Slovenia,
(16) Saint Martin's University, Lacey, USA,
(17) Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, France,
(18) Leibniz Institut für Astrophysik Potsdam, Germany)
http://arxiv.org/abs/1802.07658
The Updated BaSTI Stellar Evolution Models and Isochrones: I. Solar Scaled Calculations. (arXiv:1802.07319v1 [astro-ph.GA])
Volume 13, Issue 8 - article #14
S. L. Hidalgo
(1, 2),
A. Pietrinferni
(3),
S. Cassisi
(3),
M. Salaris
(4),
A. Mucciarelli
(5, 6),
A. Savino
(4, 7),
A. Aparicio
(1, 2),
V. Silva Aguirre
(8),
K. Verma
(8)
((1) Instituto de Astrofísica de Canarias,
(2) Department of Astrophysics of University of La Laguna,
(3) INAF-Osservatorio Astronomico d'Abruzzo,
(4) Astrophysics Research Institute Liverpool John Moores University,
(5) Dipartimento di Fisica e Astronomia - Universitá a degli Studi di Bologna,
(6) INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna,
(7) Kapteyn Astronomical Institute University of Groningen,
(8) Stellar Astrophysics Centre Department of Physics, Astronomy Aarhus University)
http://arxiv.org/abs/1802.07319
On the RR Lyrae stars in globulars: V. the complete Near-Infrared (JHKs) census of omega Centauri RR Lyrae variables. (arXiv:1802.03578v1 [astro-ph.SR])
Volume 13, Issue 7 - article #7
V. F. Braga
(1, 2, 3, 4),
P. B. Stetson
(5),
G. Bono
(3, 6),
M. Dall'Ora
(7),
I. Ferraro
(6),
G. Fiorentino
(8),
G. Iannicola
(6),
M. Marconi
(7),
M. Marengo
(9),
A. J. Monson
(10),
J. Neeley
(9),
S. E. Persson
(10),
R. L. Beaton
(10),
R. Buonanno
(3, 11),
A. Calamida
(12),
M. Castellani
(6),
E. Di Carlo
(11),
M. Fabrizio
(4),
W. L. Freedman
(13),
L. Inno
(14),
B. F. Madore
(10),
D. Magurno
(3),
E. Marchetti
(15),
S. Marinoni
(4),
P. Marrese
(4),
N. Matsunaga
(16),
D. Minniti
(1, 2, 17),
M. Monelli
(18),
M. Nonino
(19),
A. M. Piersimoni
(11),
A. Pietrinferni
(11),
P. Prada-Moroni
(20, 21),
L. Pulone
(6),
R. Stellingwerf
(22),
E. Tognelli
(20, 21),
A. R. Walker
(23),
E. Valenti
(15),
M. Zoccali
(1, 24)
((1) Instituto Milenio de Astrofisica, Santiago, Chile,
(2) Departamento de Fisica, Facultad de Ciencias Exactas, Universidad Andres Bello, Santiago, Chile,
(3) Department of Physics, Università di Roma Tor Vergata, Roma, Italy,
(4) SSDC, Roma, Italy,
(5) NRC-Herzberg, Dominion Astrophysical Observatory, Victoria, Canada,
(6) INAF-Osservatorio Astronomico di Roma, Monte Porzio Catone, Italy,
(7) INAF-Osservatorio Astronomico di Capodimonte, Napoli, Italy,
(8) INAF-Osservatorio Astronomico di Bologna, Bologna, Italy,
(9) Department of Physics, Astronomy, Iowa State University, Ames, IA, USA,
(10) The Observatories of the Carnegie Institution for Science, Pasadena, CA, USA,
(11) INAF-Osservatorio Astronomico d'Abruzzo, Teramo, Italy,
(12) National Optical Astronomy Observatory, Tucson AZ, USA,
(13) Department of Astronomy & Astrophysics, University of Chicago, Chicago, IL, USA,
(14) Max Planck Institute for Astronomy, Heidelberg, Germany,
(15) European Southern Observatory, Garching bei Munchen, Germany,
(16) Kiso Observatory, Institute of Astronomy, School of Science, The University of Tokyo, Kiso-machi, Japan,
(17) Vatican Observatory, Vatican City State, Italy,
(18) Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain,
(19) INAF, Osservatorio Astronoico di Trieste, Trieste, Italy,
(20) INFN, Sezione di Pisa, Pisa, Italy,
(21) Dipartimento di Fisica "Enrico Fermi", Università di Pisa, Pisa, Italy,
(22) Stellingwerf Consulting, Huntsville, AL, USA,
(23) Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, La Serena, Chile,
(24) Pontificia Universidad Catolica de Chile, Instituto de Astrofisica, Santiago, Chile)
http://arxiv.org/abs/1802.03578
Chemical analysis of eight giant stars of the globular cluster NGC 6366. (arXiv:1801.09968v1 [astro-ph.GA])
Volume 13, Issue 5 - article #2
Arthur A. Puls
(1),
Alan Alves-Brito
(1),
Fabíola Campos
(2),
Bruno Dias
(3),
Beatriz Barbuy
(4)
((1) Departamento de Astronomia -- Universidade Federal do Rio Grande do Sul -- Porto Alegre -- Brazil,
(2) Department of Astronomy -- University of Texas at Austin -- Austin -- USA,
(3) European Southern Observatory -- Santiago -- Chile,
(4) Universidade de São Paulo -- IAG -- São Paulo -- Brazil)
http://arxiv.org/abs/1801.09968
The HST large programme on $omega$ Centauri - II. internal kinematics. (arXiv:1801.01504v1 [astro-ph.GA])
Volume 13, Issue 2 - article #17
A. Bellini
(1),
M. Libralato
(1),
L. R. Bedin
(2),
A. P. Milone
(3),
R. P. van der Marel
(1,4),
J. Anderson
(1),
D. Apai
(5.6),
A. J. Burgasser
(7),
A. F. Marino
(8),
J. M. Rees
(5)
((1) STScI,
(2) INAF-OAPD,
(3) UNIPD,
(4) JHU,
(5) Astronomy Dept., The University of Arizona
(6) Lunar, Planetary Obs, The University of Arizona,
(7) UCSD,
(8) Australian National University)
http://arxiv.org/abs/1801.01504
J0811+4730: the most metal-poor star-forming dwarf galaxy known. (arXiv:1709.00202v1 [astro-ph.GA])
Volume 12, Issue 36 - article #2
Y. I. Izotov
(1),
T. X. Thuan
(2),
N. G. Guseva
(1),
S. E. Liss
(2)
((1) Main Astronomical Observatory, Ukrainian National Academy of Sciences, Kyiv, Ukraine,
(2) Astronomy Department, University of Virginia, Charlottesville, USA)
http://arxiv.org/abs/1709.00202
Observing the metal-poor solar neighbourhood: a comparison of galactic chemical evolution predictions. (arXiv:1705.03642v1 [astro-ph.SR])
Volume 12, Issue 19 - article #2
T. Mishenina
(1),
M. Pignatari
(2,3,6),
B.Cot'e
(3,4,5,6),
F.-K. Thielemann
(7),
C. Soubiran
(8),
N. Basak
(1),
T. Gorbaneva
(1),
S.A. Korotin
(1,9),
V.V. Kovtyukh
(1),
B. Wehmeyer
(7),
S. Bisterzo
(3,10,11),
C. Travaglio
(3,10,11),
B.K. Gibson
(2,6),
C. Jordan
(2,6),
A. Paul
(4),
C. Ritter
(3,6),
F. Herwig
(3,6)
((1) Astronomical Observatory, Odessa National University,, Isaac Newton Institute of Chile, Odessa branch, Odessa, Ukraine,
(2) E.A. Milne Centre for Astrophysics, University of Hull,
(3) The NuGrid Collaboration,
(4) Department of Physics, Astronomy, University of Victoria,
(5) National Superconducting Cyclotron Laboratory, Michigan State University,
(6) Joint Institute for Nuclear Astrophysics Center for the Evolution of the Elements,
(7) Department of Physics, University of Basel,
(8) Laboratoire d'Astrophysique de Bordeaux, Univ. Bordeaux - CNRS, B18N, allée Geoffroy Saint-Hilaire,
(9) Crimean Astrophysical Observatory,
(10) INAF, Astrophysical Observatory Turin, Strada Osservatorio 20,
(11) B2FH Association)
http://arxiv.org/abs/1705.03642
The binarity of Galactic dwarf stars along with effective temperature and metallicity. (arXiv:1703.10305v1 [astro-ph.SR])
Volume 12, Issue 13 - article #3
Shuang Gao
(1),
He Zhao
(1),
Hang Yang
(1),
Ran Gao
(1)
((1) Department of Astronomy, Beijing Normal University)
http://arxiv.org/abs/1703.10305
Gaia 1 and 2. A pair of new satellites of the Galaxy. (arXiv:1702.01122v1 [astro-ph.GA])
Volume 12, Issue 6 - article #4
S. E. Koposov
(1),
V. Belokurov
(1),
G. Torrealba
(1)
((1) Institute of Astronomy, University of Cambridge)
http://arxiv.org/abs/1702.01122
Chemical characterization of the globular cluster NGC 5634 associated to the Sagittarius dwarf spheroidal galaxy. (arXiv:1701.03116v1 [astro-ph.SR])
Volume 12, Issue 2 - article #1
Eugenio Carretta
(1),
Angela Bragaglia
(1),
Sara Lucatello
(2),
Valentina D'Orazi
(2,3,4),
Raffaele G. Gratton
(2),
Paolo Donati
(1,5),
Antonio Sollima
(1),
Chris Sneden
(6)
((1) INAF-Osservatorio Astronomico di Bologna,
(2) INAF-Osservatorio Astronomico di Padova,
(3) Dept. of Physics, Astronomy, Macquarie Univ.,
(4) Monash Centre for Astrophysics,
(5) DIFA, Universita' di Bologna,
(6) Dept. of Astronomy, McDonald Observatory, The University of Texas, Austin, USA)
http://arxiv.org/abs/1701.03116
Metallicities in the Outer Regions of Spiral Galaxies. (arXiv:1612.05278v1 [astro-ph.GA])
Volume 11, Issue 52 - article #3
Fabio Bresolin
(Institute for Astronomy, University of Hawaii)
http://arxiv.org/abs/1612.05278
Pan-STARRS Photometric and Astrometric Calibration. (arXiv:1612.05242v1 [astro-ph.IM])
Volume 11, Issue 51 - article #5
Eugene. A. Magnier
(1),
Edward. F. Schlafly
(2,3),
Douglas P. Finkbeiner
(4,5),
J. L. Tonry
(1),
B. Goldman
(6),
S. Röser
(7),
E. Schilbach
(7),
K. C. Chambers
(1),
H. A. Flewelling
(1),
M. E. Huber
(1),
P. A. Price
(8),
W. E. Sweeney
(1),
C. Z. Waters
(1),
L. Denneau
(1),
P. Draper
(9),
K. W. Hodapp
(1),
R. Jedicke
(1),
R.-P. Kudritzki
(1),
N. Metcalfe
(9),
C. W. Stubbs
(10),
R. J. Wainscoast
(1)
((1) UH Institute for Astronomy,
(2) Lawrence Berkeley National Laboratory,
(3) Hubble Fellow,
(4) ITC Harvard-Smithsonian Center for Astrophysics,
(5) Department of Physics Harvard University,
(6) Max Planck Institute for Astronomy,
(7) Astronomisches Rechen-Institut Zentrum für Astronomie der Universität Heidelberg,
(8) Department of Astrophysical Sciences Princeton University,
(9) Department of Physics Durham University,
(10) Harvard-Smithsonian Center for Astrophysics)
http://arxiv.org/abs/1612.05242
On the dearth of ultra-faint extremely metal poor galaxies. (arXiv:1612.00273v1 [astro-ph.GA])
Volume 11, Issue 49 - article #8
J. Sanchez Almeida
(1, 2),
M. E. Filho
(1, 2,, 3),
C. Dalla Vecchia
(1, 2),
E. D. Skillman
(4)
((1) Instituto de Astrofisica de Canarias, La Laguna, Tenerife, Spain,
(2) Departamento de Astrofisica, Universidad de La Laguna,
(3) SIM/FEUP, Porto, Portugal,
(4) Minnesota Institute for Astrophysics, School of Physics, Astronomy, University of Minnesota, Minneapolis, USA.)
http://arxiv.org/abs/1612.00273
Chemical analysis of a carbon-enhanced very metal-poor star: CD-27 14351. (arXiv:1611.01637v1 [astro-ph.SR])
Volume 11, Issue 46 - article #4
Drisya Karinkuzhi
(1),
Aruna Goswami
(1),
Thomas Masseron
(2)
((1) Indian Institute of Astrophysics, Koramangala, Bangalore 560034,
(2) Institute of Astronomy, Madingley Road, Cambridge CB3 0HA, UK)
http://arxiv.org/abs/1611.01637
Estimating distances from parallaxes. III. Distances of two million stars in the Gaia DR1 catalogue. (arXiv:1609.07369v1 [astro-ph.GA])
Volume 11, Issue 40 - article #5
Tri L. Astraatmadja
(1,2),
Coryn A. L. Bailer-Jones
(2)
((1) Department of Terrestrial Magnetism, Carnegie Institution for Science, Washington, DC,
(2) Max Planck Institute for Astronomy, Heidelberg, Germany)
http://arxiv.org/abs/1609.07369
On the RR Lyrae stars in globulars: IV. $omega$ Centauri Optical UBVRI Photometry. (arXiv:1609.04916v1 [astro-ph.SR])
Volume 11, Issue 39 - article #12
V. F. Braga
(1, 2),
P. B. Stetson
(3),
G. Bono
(1, 4),
M. Dall'Ora
(5),
I. Ferraro
(4),
G. Fiorentino
(6),
L. M. Freyhammer
(7),
G. Iannicola
(4),
M. Marengo
(8),
J. Neeley
(8),
E. Valenti
(9),
R. Buonanno
(1, 10),
A. Calamida
(11),
M. Castellani
(4),
R. da Silva
(4, 2),
S. Degl'Innocenti
(12, 13),
A. Di Cecco
(10),
M. Fabrizio
(10, 2),
W. L. Freedman
(14),
G. Giuffrida
(4, 2),
J. Lub
(15),
B. F. Madore
(16),
M. Marconi
(5),
S. Marinoni
(4, 2),
N. Matsunaga
(17),
M. Monelli
(18),
S. E. Persson
(16),
A. M. Piersimoni
(10),
A. Pietrinferni
(10),
P. Prada-Moroni
(12, 13),
L. Pulone
(4),
R. Stellingwerf
(19),
E. Tognelli
(12, 13),
A. R. Walker
(20)
((1) Department of Physics, Università di Roma Tor Vergata
(2) ASDC
(3) NRC-Herzberg, Dominion Astrophysical Observatory
(4) INAF-Osservatorio Astronomico di Roma
(5) INAF-Osservatorio Astronomico di Capodimonte
(6) INAF-Osservatorio Astronomico di Bologna
(7) Jeremiah Horrocks Institute of Astrophysics, University of Central Lancashire
(8) Department of Physics, Astronomy, Iowa State University
(9) European Southern Observatory
(10) INAF-Osservatorio Astronomico di Teramo
(11) National Optical Astronomy Observatory
(12) INFN, Sezione di Pisa
(13) Dipartimento di Fisica Enrico Fermi, Università di Pisa
(14) Department of Astronomy & Astrophysics, University of Chicago
(15) Sterrewacht Leiden, Leiden University
(16) The Observatories of the Carnegie Institution for Science
(17) Kiso Observatory, Institute of Astronomy, School of Science, The University of Tokyo
(18) Instituto de Astrofísica de Canarias
(19) Stellingwerf Consulting
(20) Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory)
http://arxiv.org/abs/1609.04916
The evolution of the Milky Way: New insights from open clusters. (arXiv:1609.02619v1 [astro-ph.GA])
Volume 11, Issue 38 - article #10
Arumalla B. S. Reddy
(1),
David L. Lambert
(1),
Sunetra Giridhar
(2)
((1) W.J. McDonald Observatory, Department of Astronomy, The University of Texas at Austin
(2) Indian Institute of Astrophysics)
http://arxiv.org/abs/1609.02619
The Age and Distance of the Kepler Open Cluster NGC 6811 from an Eclipsing Binary, Turnoff Star Pulsation, and Giant Asteroseismology. (arXiv:1608.03917v1 [astro-ph.SR])
Volume 11, Issue 34 - article #7
Eric L. Sandquist
(San Diego State University),
J. Jessen-Hansen
(Aarhus University),
Matthew D. Shetrone
(McDonald Observatory),
Karsten Brogaard
(Aarhus University),
Soren Meibom
(Harvard-Smithsonian Center for Astrophysics),
Marika Leitner
(Humboldt State University),
Dennis Stello
(Sydney Institute for Astronomy),
Hans Bruntt
(Aarhus University),
Victoria Antoci
(Aarhus University),
Jerome A. Orosz
(San Diego State University),
Frank Grundahl
(Aarhus University),
Soren Frandsen
(Aarhus University)
http://arxiv.org/abs/1608.03917
The primordial deuterium abundance of the most metal-poor damped Lyman-alpha system. (arXiv:1607.03900v1 [astro-ph.CO])
Volume 11, Issue 29 - article #5
Ryan Cooke
(1),
Max Pettini
(2,3),
Kenneth M. Nollett
(4),
Regina Jorgenson
(5,6),
((1) University of California, Santa Cruz,
(2) Institute of Astronomy, University of Cambridge,
(3) Kavli Institute for Cosmology, University of Cambridge,
(4) San Diego State University,
(5) Willamette University,
(6) Maria Mitchell Observatory)
http://arxiv.org/abs/1607.03900
The extended halo of Centaurus A: uncovering satellites, streams and substructures
Volume 10, Issue 46 - article #17
D. Crnojević
,
(1),
D. J. Sand
(1),
K. Spekkens
(2),
N. Caldwell
(3),
P. Guhathakurta
(4),
B. McLeod
(3),
A. Seth
(5),
J. Simon
(6),
J. Strader
(7),
E. Toloba
(1,4)
((1) Department of Physics, Texas Tech University, Lubbock, TX, USA,
(2) Department of Physics, Royal Military College of Canada, Kingston, Ontario, Canada,
(3) Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA,
(4) UCO/Lick Observatory, University of California, Santa Cruz, CA, USA,
(5) Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA,
(6) Observatories of the Carnegie Institution for Science, Pasadena, CA, USA,
(7) Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA)
arXiv.org - Astrophysics - Volume: 2015, Issue: 18 Dec
arXiv:1512.05366
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Resolving the extended stellar halos of nearby galaxies: the wide-field PISCeS survey
Volume 10, Issue 38 - article #7
D. Crnojević
,
(1),
D. J. Sand
(1),
N. Caldwell
(2),
P. Guhathakurta
(3),
B. McLeod
(2),
A. Seth
(4),
J. D. Simon
(5),
J. Strader
(6),
E. Toloba
(1,3)
((1) Texas Tech University, Physics Department, Lubbock, TX, USA,
(2) Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA,
(3) UCO/Lick Observatory, University of California, Santa Cruz, CA, USA,
(4) Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA,
(5) Observatories of the Carnegie Institution for Science, Pasadena, CA, USA,
(6) Michigan State University, Department of Physics and Astronomy, East Lansing, MI, USA)
arXiv.org - Astrophysics - Volume: 2015, Issue: 16 Oct
arXiv:1510.03487
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The Primordial Abundance of Deuterium: Ionization correction
Volume 10, Issue 38 - article #9
Ryan Cooke
(1),
Max Pettini
(2),
((1) University of California, Santa Cruz,
(2) Institute of Astronomy, University of Cambridge)
arXiv.org - Astrophysics - Volume: 2015, Issue: 16 Oct
arXiv:1510.03867
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Vertical kinematics of the thick disc at 4.5 < R < 9.5 kpc
Volume 10, Issue 30 - article #15
Kohei Hattori
,
Gerard Gilmore
(Institute of Astronomy, Cambridge, UK)
arXiv.org - Astrophysics - Volume: 2015, Issue: 21 Aug
arXiv:1508.04429
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Local associations and the barium puzzle
Volume 10, Issue 29 - article #4
Arumalla B. S. Reddy
(1),
David L. Lambert
(1)
((1) W.J. McDonald Observatory and Department of Astronomy, The University of Texas at Austin)
arXiv.org - Astrophysics - Volume: 2015, Issue: 14 Aug
arXiv:1508.02815
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Grid Search in Stellar Parameters: a software for spectrum analysis of single stars and binary systems
Volume 10, Issue 25 - article #19
Andrew Tkachenko
(Institute of Astronomy, KU Leuven)
arXiv.org - Astrophysics - Volume: 2015, Issue: 17 Jul
arXiv:1507.02864
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Discovery of low-metallicity stars in the central parsec of the Milky Way
Volume 10, Issue 25 - article #23
Tuan Do
(1 and 2),
Wolfgang Kerzendorf
(3 and 4),
Nathan Winsor
(1 and 5),
Morten Støstad
(3),
Mark R. Morris
(2),
Jessica R. Lu
(6),
Andrea M. Ghez
(2)
((1) Dunlap Institute, University of Toronto,
(2) Physics and Astronomy Department, UCLA,
(3) Department of Astronomy, University of Toronto,
(4) ESO,
(5) Grenfell Campus, Memorial University of Newfoundland,
(6) IfA, University of Hawaii)
arXiv.org - Astrophysics - Volume: 2015, Issue: 3 Jul
arXiv:1506.07891
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Chemical abundances of giant stars in the Crater stellar system
Volume 10, Issue 23 - article #4
P. Bonifacio
(1),
E. Caffau
(1),
S. Zaggia
(2),
P. François
(1,3),
L. Sbordone
(4,5),
S.M. Andrievsky
(6,1),
S.A. Korotin
(6)
((1) GEPI, Observatoire de Paris, CNRS, Univ Paris Diderot
(2) INAF-OAPD,
(3) UPJV,
(4) MIA, Chile,
(5) PUC, Chile,
(6) Department of Astronomy and Astronomical Observatory, Odessa National University, and Isaac Newton Institute of Chile Odessa branch)
arXiv.org - Astrophysics - Volume: 2015, Issue: 12 Jun
arXiv:1506.03615
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Understanding AGB evolution in Galactic bulge stars from high-resolution infrared spectroscopy
Volume 10, Issue 18 - article #18
S. Uttenthaler
(1),
J. A. D. L. Blommaert
(2,3),
P. R. Wood
(4),
T. Lebzelter
(1),
B. Aringer
(5,1),
M. Schultheis
(6),
N. Ryde
(7)
((1) University of Vienna, Department of Astrophysics,
(2) Department of Physics and Astrophysics, Vrije Universiteit Brussel,
(3) Instituut voor Sterrenkunde, KU Leuven,
(4) Research School of Astronomy and Astrophysics, Australian National University,
(5) Department of Physics and Astronomy G. Galilei, University of Padova,
(6) Laboratoire Lagrange, Université de Nice Sophia Antipolis,
(7) Lund Observatory, Sweden)
arXiv.org - Astrophysics - Volume: 2015, Issue: 8 May
arXiv:1505.01425
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TOPoS: II. On the bimodality of carbon abundance in CEMP stars. Implications on the early chemical evolution of galaxies
Volume 10, Issue 16 - article #19
P. Bonifacio
(1),
E. Caffau
(1,2),
M. Spite
(2),
M. Limongi
(3,4),
A. Chieffi
(5),
R.S. Klessen
(6,7,8),
P. François
(1,9),
P. Molaro
(10),
H. G. Ludwig
(2,1),
S. Zaggia
(11),
F. Spite
(1),
B. Plez
(12),
R. Cayrel
(1),
N. Christlieb
(2),
P.C. Clark
(13,6),
S.C.O. Glover
(6),
F. Hammer
(1),
A. Koch
(2),
L. Monaco
(14,15),
L. Sbordone
(16,17),
M. Steffen
(18,1)
((1) GEPI, Observatoire de Paris,
(2) ZAH-LSW,
(3) INAF - OA Roma,
(4) Kavli IPMU, Univ. Tokyo
(5) INAF - IASFC,
(6) ZAH-ARI,
(7) Kavli, IPAC, Stanford Univ.,
(8) Dep A&A Univ, Calfornia,
(9) UPJV, Univ. Picardie,
(10) INAF - OA Trieste,
(11) INAF- OA Padova,
(12) LUPM, Univ. Montpellier,
(13) School of Physics and Astronomy, Cardiff Univ.
(14) ESO,
(15) DCF - Univ. A. Bello,
(16) MAS,
(17) PUC - Chile,
(18) Leibniz-Institut AIP)
arXiv.org - Astrophysics - Volume: 2015, Issue: 24 Apr
arXiv:1504.05963
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Kinematics and Velocity Ellipsoid of the Solar Neighborhood White Dwarfs
Volume 10, Issue 10 - article #8
W. H. Elsanhoury
,
M. I. Nouh
,
H. I. Abdel-Rahman
(Department of Astronomy, National Research Institute of Astronomy and Geophysics, Cairo, Egypt)
arXiv.org - Astrophysics - Volume: 2015, Issue: 13 Mar
arXiv:1503.03595
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The VLT Survey Telescope ATLAS
Volume 10, Issue 7 - article #9
T. Shanks
(1),
N. Metcalfe
(1),
B. Chehade
(1),
J.R. Findlay
(1),
M.J. Irwin
(2),
E. Gonzalez-Solares
(2),
J.R. Lewis
(2),
A. Kupcu Yoldas
(2),
R.G.Mann
(3),
M.A. Read
(3),
E.T.W. Sutorius
(3),
S. Voutsinas
(3)
((1) Dept of Physics, Durham University, UK,
(2) Institute of Astronomy, University of Cambridge, UK
(3) Institute for Astronomy, University of Edinburgh, UK)
arXiv.org - Astrophysics - Volume: 2015, Issue: 20 Feb
arXiv:1502.05432
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The origin and evolution of the odd-Z iron-peak elements Sc, V, Mn, and Co in the Milky Way stellar disk
Volume 10, Issue 5 - article #9
Chiara Battistini
(1),
Thomas Bensby
(1)
((1) Lund Observatory, Department of Astronomy and Theoretical Physics, Lund, Sweden)
arXiv.org - Astrophysics - Volume: 2015, Issue: 6 Feb
arXiv:1502.01152
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A search for open cluster Cepheids in the Galactic plane
Volume 9, Issue 23 - article #11
Xiaodian Chen
(1,2,3),
Richard de Grijs
(1,2),
Licai Deng
(3)
((1) Kavli Institute for Astronomy and Astrophysics, Peking University
(2) Department of Astronomy, Peking University
(3) Key Laboratory for Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences)
arXiv.org - Astrophysics - Volume: 2014, Issue: 17 Oct
arXiv:1410.4489
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Properties of the Young Milky Way Globular Cluster Whiting 1 from Near-Infrared Photometry
Volume 9, Issue 23 - article #18
A. T. Valcheva
(1),
E. P. Ovcharov
(1),
A. D. Lalova
(2),
P. L. Nedialkov
(1),
V. D. Ivanov
(3),
G. Carraro
(3)
((1) Department of Astronomy, University of Sofia,
(2) Institute of Optical Materials and Technologies, BAS,
(3) European Southern Observatory)
arXiv.org - Astrophysics - Volume: 2014, Issue: 17 Oct
arXiv:1410.3419
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Searching for Chemical Signatures of Multiple Stellar Populations in the Old, Massive Open Cluster NGC 6791
Volume 9, Issue 23 - article #30
A. Bragaglia
(1),
C. Sneden
(2,3,4),
E. Carretta
(1),
R.G. Gratton
(4),
S. Lucatello
(4),
P.F. Bernath
(5),
J.S.A. Brooke
(6),
R.S. Ram
(6)
(1-INAF OA Bologna, 2-Dept. Astronomy & McDonals Obs. Austin, TX, 3-Ege Univ. Izmir, 4-INAF OA Padova, 5-Old Dominion Univ. Norfolk, VA, 6-Univ. of York)
arXiv.org - Astrophysics - Volume: 2014, Issue: 3 Oct
arXiv:1409.8283
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Nitrogen abundances and multiple stellar populations in the globular clusters of the Fornax dSph
Volume 9, Issue 22 - article #42
S. S. Larsen
(1),
J. P. Brodie
(2),
F. Grundahl
(3),
J. Strader
(4)
((1) Department of Astrophysics/IMAPP, Radboud University Nijmegen, The Netherlands,
(2) UCO/Lick Observatory, UC Santa Cruz, USA,
(3) Stellar Astrophysics Centre, Aarhus University, Denmark,
(4) Department of Physics and Astronomy, Michigan State University, USA)
arXiv.org - Astrophysics - Volume: 2014, Issue: 5 Sep
arXiv:1409.0541
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other
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The Milky Way as a High Redshift Galaxy: The Importance of Thick Disk Formation in Galaxies
Volume 9, Issue 20 - article #24
Matthew D. Lehnert
(1),
Paola Di Matteo
(2),
Misha Haywood
(2),
Owain N. Snaith
(3)
((1) Institut d'Astrophysique de Paris,
(2) GEPI, Observatoire de Paris,
(3) Department of Physics & Astronomy, University of Alabama)
arXiv.org - Astrophysics - Volume: 2014, Issue: 13 Jun
arXiv:1406.3039
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The most metal-poor damped Lyman alpha systems: An insight into dwarf galaxies at high redshift
Volume 9, Issue 20 - article #130
Ryan Cooke
(1),
Max Pettini
(2),
Regina A. Jorgenson
(3),
((1) University of California, Santa Cruz,
(2) Institute of Astronomy, University of Cambridge,
(3) Institute for Astronomy, University of Hawaii)
arXiv.org - Astrophysics - Volume: 2014, Issue: 4 Jul
arXiv:1406.7003
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Stellar Mergers Are Common
Volume 9, Issue 19 - article #6
C.S. Kochanek
(1),
Scott M. Adams
(1),
Krzysztof Belczynski
(2,3)
((1) Department of Astronomy and the Center for Cosmology and AstroParticle Physics, The Ohio State University,
(2) Astronomical Observatory, Warsaw University,
(3) Center for Gravitational Wave Astronomy, University of Texas at Brownsville)
arXiv.org - Astrophysics - Volume: 2014, Issue: 9 May
arXiv:1405.1042
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other
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Stellar Metallicity of the Extended Disk and Distance of the Spiral Galaxy NGC 3621
Volume 9, Issue 18 - article #6
Rolf-Peter Kudritzki
(1),
Miguel A. Urbaneja
(2),
Fabio Bresolin
(1),
Matthew. W. Hosek Jr
(1),
Norbert Przybilla
(2)
((1) Institute for Astronomy, University of Hawaii
(2) Institute for Astro- and Particle Physics, University of Innsbruck)
arXiv.org - Astrophysics - Volume: 2014, Issue: 2 May
arXiv:1404.7244
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Stellar laboratories III. New Ba V, Ba VI, and Ba VII oscillator strengths and the barium abundance in the hot white dwarfs G191-B2B and RE0503-289
Volume 9, Issue 17 - article #7
T. Rauch
(1),
K. Werner
(1),
P. Quinet
(2,3),
J. W. Kruk
(4)
((1) Institute for Astronomy and Astrophysics, Eberhard Karls University, Tuebingen, Germany,
(2) Astrophysique et Spectroscopie, Universite de Mons - UMONS, Belgium,
(3) IPNAS, Universite de Liege, Liege, Belgium,
(4) NASA Goddard Space Flight Center, Greenbelt, USA)
arXiv.org - Astrophysics - Volume: 2014, Issue: 25 Apr
arXiv:1404.6094
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New 2MASS Near-infrared Photometry for Globular Clusters in M31
Volume 9, Issue 16 - article #5
Song Wang
(1,2),
Jun Ma
(1),
Zhenyu Wu
(1),
Xu Zhou
(1)
((1) Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences,
(2) University of Chinese Academy of Sciences)
arXiv.org - Astrophysics - Volume: 2014, Issue: 18 Apr
arXiv:1404.4444
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Chemical composition and constraints on mass loss for globular clusters in dwarf galaxies: WLM and IKN
Volume 9, Issue 15 - article #1
S. S. Larsen
(1),
J. P. Brodie
(2),
D. A. Forbes
(3),
J. Strader
(4)
((1) Department of Astrophysics/IMAPP, Radboud University Nijmegen, The Netherlands,
(2) UCO/Lick Observatory, UC Santa Cruz, USA,
(3) Swinburne University of Technology, Australia,
(4) Department of Physics and Astronomy, Michigan State University, USA)
arXiv.org - Astrophysics - Volume: 2014, Issue: 11 Apr
arXiv:1404.1916
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Detailed AGB evolutionary models and near infrared colours of intermediate-age stellar populations: Tests on star clusters
Volume 9, Issue 11 - article #8
M. Salaris
(1,2),
A. Weiss
(2),
L. Cassara'
,
(3,4),
L. Piovan
(3),
C. Chiosi
(3)
(1- Astrophysics Research Institute, Liverpool John Moores University, UK, 2- Max-Planck-Institut fur Astrophysik, D, 3- Department of Physics and Astronomy, University of Padova, I, 4- INAF-IASF Milano, I)
arXiv.org - Astrophysics - Volume: 2014, Issue: 14 Mar
arXiv:1403.2505
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The extreme chemistry of multiple stellar populations in the metal-poor globular cluster NGC 4833
Volume 9, Issue 5 - article #13
E. Carretta
(1),
A. Bragaglia
(1),
R.G. Gratton
(2),
V. D'Orazi
(3,4),
S. Lucatello
(2),
Y. Momany
(2,5),
A. Sollima
(1),
M. Bellazzini
(1),
G. Catanzaro
(6),
F. Leone
(7)
((1) INAF-Osservatorio Astronomico di Bologna,
(2) INAF-Osservatorio Astronomico di Padova,
(3) Dept. of Physics and Astronomy, Macquarie Univ.,
(4) Monash Centre for Astrophysics,
(5) ESO,
(6) INAF-Osservatorio Astrofisico di Catania,
(7) Dip. Fisica e Astr., Univ. Catania)
arXiv.org - Astrophysics - Volume: 2014, Issue: 31 Jan
arXiv:1401.7325
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A sequence of nitrogen-rich very red giants in the globular cluster NGC 1851
Volume 9, Issue 3 - article #2
Eugenio Carretta
(1),
Valentina D'Orazi
(2,3),
Raffaele G. Gratton
(4),
Sara Lucatello
(4)
((1) INAF-Osservatorio Astronomico di Bologna,
(2) Dept. of Physics and Astronomy, Macquarie Univ.,
(3) Monash Centre for Astrophysics,
(4) INAF-Osservatorio Astronomico di Padova.)
arXiv.org - Astrophysics - Volume: 2014, Issue: 17 Jan
arXiv:1401.2986
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