Solution to the problem of the surface gravity distribution of cool da white dwarfs from improved 3D model atmospheres

Astronomy and Astrophysics

Volumn 531, Issue , 2011, Pages

  Tremblay, P E ^a   Ludwig, H G ^b   Steffen, M ^c   Bergeron, P ^a   Freytag, B ^d  

^a UNIVERSITÉ DE MONTRÉAL   (Canada)

^b UNIVERSITÄT HEIDELBERG   (Germany)

^c ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

^d UNIVERSITÉ DE LYON   (France)

Author keywords

Convection; Line: profiles; Stars: atmospheres; White dwarfs

Indexed keywords

COMPUTATION THEORY; HEAT CONVECTION; MIXING; SPECTROSCOPIC ANALYSIS;

CONVECTIVE ENERGY; DIFFERENTIAL ANALYSIS; EFFECTIVE TEMPERATURE; HYDRODYNAMICAL MODEL; HYDROGEN ATMOSPHERE; LINE: PROFILES; MIXING LENGTH THEORIES; STARS: ATMOSPHERE;

WHITE DWARFS;

EID: 79960184089     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201117310     Document Type: Article

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