The evolution of a rapidly accreting helium white dwarf to become a low-luminosity helium star

Monthly Notices of the Royal Astronomical Society

Volumn 313, Issue 4, 2000, Pages 671-677

  Saio, Hideyuki ^a   Jeffery, C Simon ^b  

^a TOHOKU UNIVERSITY   (Japan)

^b ARMAGH OBSERVATORY   (United Kingdom)

Author keywords

Stars: Chemically peculiar; Stars: Evolution; Stars: Individual: V652 Her; Stars: Oscillations

Indexed keywords

GRAVITATION; LUMINANCE; MERGING; SHELLS (STRUCTURES); WHITE DWARFS;

HELIUM-BURNING; HIGH-GRAVITY; LOW-MASS; MERGING PROCESS; PROPERTY; STAR OSCILLATIONS; STAR: EVOLUTION; STAR: INDIVIDUAL: V652 HER; STARS: CHEMICALLY PECULIAR; STARS: INDIVIDUAL: PROXIMA CENTAURI;

HELIUM;

EID: 0001370299     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2000.03221.x     Document Type: Article

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