Balmer lines as Teff and log g indicators for non-solar composition atmospheres an application to the extremely helium-weak star HR 6000

Astronomy and Astrophysics

Volumn 425, Issue 2, 2004, Pages 641-648

  Catanzaro, G ^a   Leone, F ^a   Dall, T H ^b  

^a INAF OSSERVATORIO ASTROFISICO DI CATANIA   (Italy)

^b EUROPEAN SOUTHERN OBSERVATORY   (Chile)

Author keywords

Stars: abundances; Stars: atmospheres; Stars: chemically peculiar; Stars: fundamental parameters; Stars: individual: HR 6000

Indexed keywords

ATMOSPHERIC CHEMISTRY; ATMOSPHERIC TURBULENCE; COMPOSITION; GRAVITATION; MATHEMATICAL MODELS; PHOSPHORUS; SODIUM; ULTRAVIOLET RADIATION;

STARS: ABUNDANCES; STARS: ATMOSPHERES; STARS: CHEMICALLY PECULIAR; STARS: FUNDAMENTAL PARAMETERS; STARS: INDIVIDUAL: HR 6000;

ASTROPHYSICS;

EID: 5044240743     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20040558     Document Type: Article

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