Gaia FGK benchmark stars: New candidates at low metallicities

被引：0

作者：

Hawkins, K. ^{[1
]}

Jofre, P. ^{[1
]}

Heiter, U. ^{[2
]}

Soubiran, C. ^{[3
]}

Blanco-Cuaresma, S. ^{[4
]}

Casagrande, L. ^{[5
]}

Gilmore, G. ^{[1
]}

Lind, K. ^{[6
]}

Magrini, L. ^{[7
]}

Masseron, T. ^{[1
]}

Pancino, E. ^{[7
,8
,9
]}

Randich, S. ^{[7
]}

Worley, C.C. ^{[1
]}

机构：

[1] Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge,CB30HA, United Kingdom

[2] Department of Physics and Astronomy, Uppsala University, Box 516, Uppsala,75120, Sweden

[3] Universite de Bordeaux, CNRS, Floirac,33270, France

[4] Observatoire de Geneve, Universite de Geneve, Versoix,1290, Switzerland

[5] Research School of Astronomy and Astrophysics, Australian National University, ACT,2611, Australia

[6] Max-Planck Institute for Astronomy, Konigstuhl 17, Heidelberg,69117, Germany

[7] INAF, Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, Firenze,50125, Italy

[8] INAF, Osservatorio Astronomico di Bologna, via Ranzani 1, Bologna,40127, Italy

[9] ASI, Science Data Center, via del Politecnico snc, Rome,00133, Italy

来源：

Astronomy and Astrophysics | 2016年 / 592卷

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Jofre, P.
Heiter, U.
Soubiran, C.
Blanco-Cuaresma, S.
Casagrande, L.
Gilmore, G.
Lind, K.
Magrini, L.
Masseron, T.
Pancino, E.
Randich, S.
Worley, C. C.
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[2] Gaia FGK benchmark stars: Metallicity
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