Gaia FGK benchmark stars: Opening the black box of stellar element abundance determination

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作者
Jofré, P. [1 ,2 ]
Heiter, U. [3 ]
Worley, C.C. [1 ]
Blanco-Cuaresma, S. [4 ]
Soubiran, C. [5 ]
Masseron, T. [1 ]
Hawkins, K. [1 ,6 ]
Adibekyan, V. [7 ]
Buder, S. [8 ]
Casamiquela, L. [9 ]
Gilmore, G. [1 ]
Hourihane, A. [1 ]
Tabernero, H. [10 ]
机构
[1] Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge,CB3 0HA, United Kingdom
[2] Núcleo de Astronomía, Facultad de Ingeniería, Universidad Diego Portales, Av. Ejército 441, Santiago, Chile
[3] Department of Physics and Astronomy, Uppsala University, Box 516, Uppsala,75120, Sweden
[4] Observatoire de Genève, Université de Genève, Versoix,1290, Switzerland
[5] Laboratoire d'Astrophysique de Bordeaux, Univ. Bordeaux, CNRS, UMR 5804, Pessac,33615, France
[6] Department of Astronomy, Columbia University, 550 W 120th St, New York,NY,10027, United States
[7] Instituto de Astrofísica e Ciências Do Espaço, Universidade Do Porto, CAUP, Rua das Estrelas, Porto,4150-762, Portugal
[8] Max-Planck Institute for Astronomy, Heidelberg,69117, Germany
[9] Departament d'Astronomia i Meteorologia, Universitat de Barcelona, ICC/IEEC, Barcelona,08007, Spain
[10] Dpto. Astrofísica, Facultad de CC. Físicas, Universidad Complutense de Madrid, Madrid,28040, Spain
来源
Astronomy and Astrophysics | 2017年 / 601卷
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