Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
OMP
LATT, Observatoire Midi-Pyrenees, Universite Paul Sabatier, Toulouse
Institut de Recherches en Astrophysique et Planetologie, 14 avenue Edouard Belin, 31400, Toulouse, France
LATT-UMR 5572, CNRS & Université P. Sabatier, 14 Av. E. Belin, 31400 Toulouse, France
Observatoire de Toulouse, France
Observatoire Midi-Pyrenees, Toulouse, France
Laboratoire d'Astronomie de Toulouse-Tarbes, Université de Toulouse, 14 Avenue Edouard Belin, 31400 Toulouse, France
Laboratoire d'Astrophysique de Toulouse et Tarbes, CNRS, Université de Toulouse; 14 avenue Edouard Belin, 31400 Toulouse, France
Laboratoire d'Astrophysique de Toulouse, Observatoire Midi-Pyrénées et Université Paul Sabatier, 14 avenue Edouard Belin, 31400-Toulouse, France sylvie.vauclairatast.obs-mip.fr
Laboratoire d'Astrophysique, Observatoire Midi-Pyrénées, Toulouse, France
LATT, Observatoire Midi-Pyrenees, Universite Paul Sabatier, Toulouse, France
Centre d'Études Nucleaires de Saclay
LATT-UMR 5572, CNRS & Université P. Sabatier, 14 Av. E. Belin, F-31400 Toulouse, France
Laboratoire d'Astrophysique de Toulouse-Tarbes, Université de Toulouse, CNRS, 14 av. E. Belin, 31400 Toulouse, France
Laboratoire d'Astrophysique Toulouse-Tarbes - OMP, 14 avenue Edouard Belin, 31400 Toulouse, France
Laboratoire d'Astrophysiue, Observatoire Mdi-Pyrénées, Toulouse, France
Meudon, Observatoire, Meudon, Hauts-de-Seine, Franc; New York, State University, Stony Brook, N.Y; Columbia University, New York, N.Y.
Paris, Observatoire, Meudon, Hauts-de-Seine, France; California Institute of Technology, Pasadena, Calif.
LATT, UPS, CNRS, UMR 5572, 14 Av Ed.Belin, 31 400 Toulouse, France
Meudon, Observatoire, Meudon, Hauts-de-Seine, France
LATT-UMR 5572, CNRS & Université P. Sabatier, 14 Av. E. Belin, F-31400, Toulouse, France
Columbia University, New Yor; New York, State University, Stony Brook, N.Y; Californ
2011 EX4
2D Simulation
A Metal-poor Double-lined Spectroscopic Binary With C, Li, And S-process Overabundances
A new step towards the explanation of lithium- and beryllium-deficient F stars. I - The field stars
Abundance anomalies in main-sequence stars - Competition between diffusion processes and turbulent motions
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