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Results 1 - 20 of 20
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
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
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
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 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
Classification Study of WISE Infrared Sources: Identification of Candidate Asymptotic Giant Branch Stars
Volume 7, Issue 27 - article #4
Xun Tu
,
Zhongxiang Wang
(Shanghai Astronomical Observatory, CAS, China)
arXiv.org - Astrophysics - Volume: 2012, Issue: 6 Jul
arXiv:1207.0294
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Structural Parameters for Globular Clusters in the Outer Halo of M31
Volume 7, Issue 13 - article #19
Song Wang
(1,2,3),
Jun Ma
(1,3)
((1) National Astronomical Observatories, Chinese Academy of Sciences,
(2) Graduate University of Chinese Academy of Sciences, Shijingshan District, Beijing, China,
(3) Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China)
arXiv.org - Astrophysics - Volume: 2012, Issue: 30 Mar
arXiv:1203.5588
[
pdf
,
ps
,
other
]
Age and structure parameters of a remote M31 globular cluster B514 based on HST, 2MASS, GALEX and BATC observations
Volume 6, Issue 45 - article #2
Jun Ma
(1,2),
Song Wang
(1,3),
Zhenyu Wu
(1),
Zhou Fan
(1),
Tianmeng Zhang
(1),
Jianghua Wu
(1)
((1) National Astronomical Observatories, Chinese Academy of Sciences,
(2) Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China,
(3) Graduate University of Chinese Academy of Sciences, Shijingshan District, Beijing, China)
arXiv.org - Astrophysics - Volume: 2011, Issue: 11 Nov
arXiv:1111.2380
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pdf
,
ps
,
other
]
Determination of fundamental properties of an M31 globular cluster from main-sequence photometry
Volume 5, Issue 34 - article #4
Jun Ma
(1,2),
Zhenyu Wu
(1),
Song Wang
(1,3),
Zhou Fan
(1),
Xu Zhou
(1),
Jianghua Wu
(1),
Zhaoji Jiang
(1),
Jiansheng Chen
(1)
((1) National Astronomical Observatories, Chinese Academy of Sciences,
(2) Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100012, China)
arXiv.org - Astrophysics - Volume: 2010, Issue: 20 Aug
arXiv:1008.2993
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other
]
Distance determination for RAVE stars using stellar models II: Most likely values assuming a standard stellar evolution scenario
Volume 5, Issue 31 - article #6
T. Zwitter
(1 and 2),
G. Matijeviv{c)
(1)
,
M. A. Breddels
(3)
,
M. C. Smith
(3
,
4)
,
A. Helmi
(3)
,
U. Munari
(5)
,
O. Bienaym'{e)
(6)
,
J. Binney
(7)
,
J. Bland-Hawthorn
(8)
,
C. Boeche
(9)
,
A. G. A. Brown
(10)
,
R. Campbell
(11)
,
K. C. Freeman
(12)
,
J. Fulbright
(13)
,
B. Gibson
(14)
,
G. Gilmore
(15)
,
E. K. Grebel
(16)
,
J. F. Navarro
(17)
,
Q. A. Parker
(18)
,
G. M. Seabroke
(19)
,
A. Siebert
(6)
,
A. Siviero
(5
,
9)
,
M. Steinmetz
(9)
,
F. G. Watson
(20)
,
M. Williams
(9)
,
R. F. G. Wyse
(13)
((1) University of Ljubljana
,
Faculty of Mathematics
,
Physics
,
Ljubljana
,
Slovenia}
(2) Center of excellence SPACE-SI
,
Ljubljana
,
Slovenia
,
(3) Kapteyn Astronomical Institute
,
University of Groningen
,
Groningen
,
The Netherlands
,
(4) Kavli Institute for Astronomy
,
Astrophysics
,
Peking University
,
Beijing
,
China
,
(5) INAF Astronomical Observatory of Padova
,
et al.
(36 additional authors not shown)
arXiv.org - Astrophysics - Volume: 2010, Issue: 30 Jul
arXiv:1007.4411
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]
The Masses of the Milky Way and Andromeda galaxies
Volume 5, Issue 9 - article #20
L.L. Watkins
(1),
N.W. Evans
(1),
J. An
(2)
((1)IoA, Cambridge,
(2)NAO, Beijing, China)
arXiv.org - Astrophysics - Volume: 2010, Issue: 26 Feb
arXiv:1002.4565
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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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,
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,
other
]
Properties and Chemical Evolution of the M31 Disk: Comparison with the Milky Way
Volume 3, Issue 29 - article #9
J.L. Hou
(1),
J. Yin
(1,4),
S. Boissier
(2),
N. Prantzos
(3),
R.X. Chang
(1),
L. Chen
(1)
((1)Shanghai Astronomical Observatory, CAS, China;
(2) Laboratoire d'Astrophysique de Marseille, France;
(3) Institute d'Astrophysique de Paris, CNRS, France;
(4) Graduate School, CAS, China)
arXiv.org - Astrophysics - Volume: 2008, Issue: 17 Jul
arXiv:0807.2492
[
ps
,
pdf
,
other
]
uvby-H
beta
CCD photometry and membership segregation of the open cluster NGC2682 (M67)
Volume 2, Issue 17 - article #12
L. Balaguer-Núñez
(1,2,3),
D. Galadí-Enríquez
(4),
C. Jordi
(1,5)
((1)UB Spain,
(2)SHAO
China,(3) IoA Cambridge
UK,(4) IAA
Spain,(5) IEEC Spain)
ArXiv - Astrophysics
arXiv:0704.2887
[
ps
,
pdf
,
other
]
Investigation of the single neutron exposure model for the s-process: the primary nature of the neutron source
Volume 2, Issue 9 - article #10
Kun Ma
(1),
W. Y. Cui
(1 and 2),
B. Zhang
(1)
((1) Department of Physics, Hebei Normal University, China,
(2) National Astronomical observatories, Chinese Academy of Sciences, China)
ArXiv - Astrophysics
astro-ph/0702677 [
abs
,
ps
,
pdf
,
other
]
Investigation for the puzzling abundance pattern of the neutron-capture elements in the ultra metal-poor star: CS 30322-023
Volume 2, Issue 9 - article #11
W. Y. Cui
(1 and 2),
B. Zhang
(1 and 2),
K. Ma
(1),
L. Zhang
(3)
((1) Department of Physics, Hebei Normal University, China,
(2) National Astronomical observatories, Chinese Academy of Sciences, China,
(3) Department of Modern Physics, University of Science and Technology of China, China)
ArXiv - Astrophysics
astro-ph/0702676 [
abs
,
ps
,
pdf
,
other
]
Investigation for the puzzling abundance pattern of the neutron-capture elements in the ultra metal-poor star: CS 30322-023
Volume 2, Issue 9 - article #11
W. Y. Cui
(1 and 2),
B. Zhang
(1 and 2),
K. Ma
(1),
L. Zhang
(3)
((1) Department of Physics, Hebei Normal University, China,
(2) National Astronomical observatories, Chinese Academy of Sciences, China,
(3) Department of Modern Physics, University of Science and Technology of China, China)
ArXiv - Astrophysics
astro-ph/0702676 [
abs
,
ps
,
pdf
,
other
]
The long-term survival chances of young massive star clusters
Volume 2, Issue 7 - article #19
Richard de Grijs
(1,2),
Genevieve Parmentier
(3)
((1) University of Sheffield, UK;
(2) National Astronomical Observatories, CAS, China;
(3) University of Liege, Belgium)
ArXiv - Astrophysics
astro-ph/0702337 [
abs
,
ps
,
pdf
,
other
]
Neutron-capture elements in the s- and r-process-rich stars: Constraints on neutron-capture nucleosynthesis processes
Volume 1, Issue 17 - article #12
Bo Zhang
,
Kun Ma
,
Guide Zhou
(Department of Physics, Hebei Normal University, China)
ArXiv - Astrophysics
astro-ph/0605340 [
abs
,
ps
,
pdf
,
other
]
The origin of the lead-rich stars in Galactic halo: investigation of the model parameters for the s-process
Volume 1, Issue 6 - article #9
Wenyuan Cui
(1,2),
Bo Zhang
(1,2)
((1) NAOC, China;
(2) Department of Physics, Hebei Normal University, China)
ArXiv - Astrophysics
astro-ph/0603039 [
abs
,
ps
,
pdf
,
other
]
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