BF Eridani: A cataclysmic variable with a massive white dwarf and an evolved secondary

Monthly Notices of the Royal Astronomical Society

Volumn 386, Issue 3, 2008, Pages 1366-1379

  Neustroev, V V ^a   Zharikov, S ^b  

^a NATIONAL UNIVERSITY OF IRELAND   (Ireland)

^b UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

Author keywords

Accretion, accretion discs; Binaries: close; Methods: observational; Novae, cataclysmic variables; Stars: dwarf novae; Stars: individual: BF Eridani

Indexed keywords

IRON COMPOUNDS; MAGNESIUM COMPOUNDS; SUPERNOVAE; VELOCITY;

ACCRETION: ACCRETION DISKS; BINARIES: CLOSE; CATACLYSMIC VARIABLES; METHODS:OBSERVATIONAL; NOVAE CATACLYSMIC VARIABLES; RADIAL VELOCITY; SPACE-VELOCITY; STAR: INDIVIDUAL: BF ERIDANI; STARS: DWARF NOVAE; STARS: INDIVIDUAL: PROXIMA CENTAURI;

WHITE DWARFS;

EID: 43049150412     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.12930.x     Document Type: Article

References (53)