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Results 1 - 15 of 15
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
Dynamical Relics of the Ancient Galactic Halo. (arXiv:1910.07538v1 [astro-ph.GA])
Volume 14, Issue 42 - article #1
Zhen Yuan
(1),
G.C. Myeong
(2,3),
Timothy C. Beers
(4),
N. Wyn Evans
(3),
Young Sun Lee
(5),
Projjwal Banerjee
(6),
Dmitrii Gudin
(4),
Kohei Hattori
(7),
Haining Li
(8),
Tadafumi Matsuno
(9),
Vinicius M. Placco
(4),
M. C. Smith
(1),
Devin D. Whitten
(4),
Gang Zhao
(8)
((1) SAO, Shanghai,
(2) CfA, Harvard,
(3) IoA, Cambridge,
(4) Notre Dame,
(5) Chungnam Univ, Daejeon,
(6) Indian Institute of Technology, Palakkad,
(7) CMU, Pittsburgh
(8) NAO, Beijing,
(9) NAOJ, Tokyo)
http://arxiv.org/abs/1910.07538
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 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
Structural parameters for globular clusters in M31
Volume 8, Issue 18 - article #11
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, Beijing,
(3) Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing)
arXiv.org - Astrophysics - Volume: 2013, Issue: 3 May
arXiv:1305.0364
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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
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Slicing and dicing the Milky Way disk in SDSS
Volume 6, Issue 48 - article #11
Martin C. Smith
(KIAA, Beijing),
S. Hannah Whiteoak
(IoA, Cambridge),
N. W. Evans
(IoA, Cambridge)
arXiv.org - Astrophysics - Volume: 2011, Issue: 2 Dec
arXiv:1111.6920
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pdf
,
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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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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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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]
What does the IMF really tell us about star formation?
Volume 4, Issue 44 - article #16
M.B.N. Kouwenhoven
(1),
S.P. Goodwin
(2)
((1) KIAA Beijing,
(2) University of Sheffield)
arXiv.org - Astrophysics - Volume: 2009, Issue: 30 Oct
arXiv:0910.4424
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,
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other
]
The formation of very wide binaries
Volume 4, Issue 37 - article #14
M. B. N. Kouwenhoven
(1,2),
S. P. Goodwin
(2),
Richard J. Parker
(2),
M. B. Davies
(3),
D. Malmberg
(3),
P. Kroupa
(4)
((1) KIAA Beijing,
(2) Sheffield University,
(3) Lund Observatory,
(4) AIfA Bonn)
arXiv.org - Astrophysics - Volume: 2009, Issue: 11 Sep
arXiv:0909.1225
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]
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