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Results 1 - 16 of 16
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
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
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
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
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
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
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
The Little Engines That Could? Globular Clusters Contribute Significantly to Reionization-era Star Formation. (arXiv:1711.00009v1 [astro-ph.GA])
Volume 12, Issue 44 - article #9
Michael Boylan-Kolchin
(The University of Texas at Austin)
http://arxiv.org/abs/1711.00009
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
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
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
[
pdf
,
ps
,
other
]
Atmospheric Parameters and Metallicities for 2191 stars in the Globular Cluster M4
Volume 8, Issue 46 - article #2
Luca Malavolta
(1 and 4),
Christopher Sneden
(2),
Giampaolo Piotto
(1 and 4),
Antonino P. Milone
(3),
Luigi R. Bedin
(4),
Valerio Nascimbeni
(4)
((1) Dipartimento di Fisica e Astronomia, Università di Padova, Padova, Italy,
(2) Department of Astronomy and McDonald Observatory, The University of Texas, Austin,
(3) Research School of Astronomy and Astrophysics, The Australian National University, Australia,
(4) INAF - Osservatorio Astronomico di Padova, Italy)
arXiv.org - Astrophysics - Volume: 2013, Issue: 15 Nov
arXiv:1311.2592
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pdf
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ps
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other
]
An upper limit on the sulphur abundance in HE 1327-2326
Volume 7, Issue 28 - article #1
P. Bonifacio
(1),
E. Caffau
(2,1),
K. A. Venn
(3),
D. L. Lambert
(4)
((1) GEPI-Observatoire de Paris, CNRS, Univ. Paris Diderot,
(2) Zentrum für Astronomie der Universität Heidelberg, Landessternwarte,
(3) Department of Physics & Astronomy, University of Victoria,
(4) The W. J. McDonald Observatory, The University of Texas at Austin)
arXiv.org - Astrophysics - Volume: 2012, Issue: 13 Jul
arXiv:1207.1806
[
pdf
,
ps
,
other
]
The VIRUS-P Exploration of Nearby Galaxies (VENGA): Survey Design and First Results
Volume 5, Issue 5 - article #11
Guillermo A. Blanc
(1),
Karl Gebhardt
(1),
Amanda Heiderman
(1),
Neal J. Evans II
(1),
Shardha Jogee
(1),
Remco van den Bosch
(1),
Irina Marinova
(1),
Tim Weinzirl
(1),
Peter Yoachim
(1),
Niv Drory
(2),
Maximilian Fabricius
(2),
David Fisher
(1),
Lei Hao
(3),
Phillip J. MacQueen
(4),
Juntai Shen
(3),
Gary J. Hill
(4),
John Kormendy
(1)
((1) Department of Astronomy, The University of Texas at Austin, Austin, USA;
(2) Max-Planck-Institut fur extraterrestrische Physik, Garching, Germany;
(3) Shanghai Astronomical Observatory, Shanghai, China;
(4) McDonald Observatory, The University of Texas at Austin, Austin, USA)
arXiv.org - Astrophysics - Volume: 2010, Issue: 29 Jan
arXiv:1001.5035
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The Abundances of Oxygen and Carbon in the Solar Photosphere
Volume 2, Issue 8 - article #9
Carlos Allende Prieto
(The University of Texas at Austin)
ArXiv - Astrophysics
astro-ph/0702429 [
abs
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other
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The First Extrasolar Planet Discovered with a New Generation High Throughput Doppler Instrument
Volume 1, Issue 16 - article #19
Jian Ge
,
Julian van Eyken
,
Suvrath Mahadevan
,
Curtis DeWitt
,
Stephen R. Kane
,
Roger Cohen
,
Andrew Vanden Heuvel
,
Scott W. Fleming
,
Pengcheng Guo
(The University of Florida),
Gregory W. Henry
(Tennessee State University),
Donald P. Schneider
,
Lawrence W. Ramsey
(The Pennsylvania State University),
Robert A. Wittenmyer
,
Michael Endl
,
William D. Cochran
(The University of Texas),
Eric B. Ford
(The University of California at Berkeley),
Eduardo L. Martin
,
Garik Israelian
(Instituto de Astrofisica de Canarias, Spain),
Jeff Valenti
(Space Telescope Science Institute),
David Montes
(Universidad Complutense de Madrid, Spain)
ArXiv - Astrophysics
astro-ph/0605247 [
abs
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ps
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other
]
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