Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
ENS-Lyon
Ecole Normale Supérieure de Lyon - CRAL - France;
Ecole Normale Superieure, Lyon
Ecole Normale Superieure de Lyon, CRAL
CRAL, ENS-Lyon
ENS-Lyon, CRAL;
Ecole Normale Superieure de Lyon, C.R.A.L
ENS Lyon, France
Ecole Normale Superieure, Lyon; Visiting Miller Professor, UC Berkeley
Centre de Recherche Astrophysique de Lyon
CRAL, Ecole Normale Superieure de Lyon;
CRAL, ENS-Lyon;
ENS-Lyon, CRAL - UMR CNRS
CRAL-ENS Lyon
C.R.A.L., France
ENSL
École Normale Supérieure de Lyon, CRAL
École Normale Superieure de Lyon, CRAL, France
Department of Physics and Astronomy, University of Rochester, Rochester, NY 14627, USA
CRAL / ENS Lyon, France
CNRS, Lyon, France
California, University, Santa Barbara
Lyon
Groupe d'Astrophysique, École Normale Supérieure de Lyon
Laboratoire de Physique, Lyon, France
Observatoire de la Cote d'Azur, Nice, France
École Normale Superieure de Lyon, France
Rochester, University, NY
Ecole Normale Supérieure de Lyon, France
ENS Lyon France
Ecole Normale Superieure de Lyon
CRAL, Ecole Normale Superieure, Lyon, France
CRAL Lyon
Ecole Normale Supérieure de Lyon - CRAL - France
Ecole Normale Supérieure, Lyon
CRAL, France
C.R.A.L., Ecole Normale Supérieure de Lyon, Lyon, France
Centre de Recherche Astronomique de Lyon
École Normale Supérieure de Lyon, 46 allée d'Italie, F-69364 Lyon cedex 07, France; Université Lyon 1, Villeurbanne, F-69622, France; CNRS, UMR 5574, Centre de Recherche Astrophysique de Lyon;
ENS-Lyon, France
École Normale Superieure de Lyon, C.R.A.L., 46 Allee d'Italie, 69364 Lyon Cedex 07, France
École Normale Superieure de Lyon, Laboratoire de Physique
École Normale Supérieure, Lyon
Lyon, École Normale Superieure, France
CRAL, École Normale Supérieure de Lyon, France
Lyon, École Normale Superieure, Lyons, France
A New Equation of State for Dense Hydrogen
A new vision on giant planet interiors: the impact of double diffusive convection
A simple method to compute white dwarf luminosity functions.
A Theory of Extrasolar Giant Planets
Activity in Very Cool Stars: Magnetic Dissipation in late-M and L Dwarf Atmospheres
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