A detached double degenerate with a 1.4-h orbital period

Monthly Notices of the Royal Astronomical Society

Volumn 288, Issue 2, 1997, Pages 538-544

  Moran, C ^a   Marsh, T R ^a   Bragaglia, A ^b  

^a UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

^b INAF OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

Author keywords

Binaries: close; Stars: individual: WD 0957 666; Supernovae: general; White dwarfs

Indexed keywords

SUPERNOVAE;

BINARIES: CLOSE; D ORBITALS; GRAVITATIONAL RADIATION; LOW-MASS; MASS RATIO; ORBITAL PERIODS; SHORT PERIODS; STAR: INDIVIDUAL: WD 0957 666; STARS: INDIVIDUAL: PROXIMA CENTAURI; SUPERNOVAE: GENERAL;

WHITE DWARFS;

EID: 0000285723     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/288.2.538     Document Type: Article

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