The mass of the white dwarf in the old nova BT Mon

Monthly Notices of the Royal Astronomical Society

Volumn 296, Issue 3, 1998, Pages 465-482

  Smith, D A ^a,b   Dhillon, V S ^c   Marsh, T R ^d  

^a UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^b ROYAL GREENWICH OBSERVATORY   (United Kingdom)

^c UNIVERSITY OF SHEFFIELD   (United Kingdom)

^d UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

Author keywords

Accretion, accretion discs; Binaries: eclipsing; Binaries: spectroscopic; Novae, cataclysmic variables; Stars: individual: BT Mon

Indexed keywords

SHEAR WAVES; VELOCITY;

ACCRETION: ACCRETION DISKS; BINARIES: SPECTROSCOPIC; BINARIES:ECLIPSING; NOVAE CATACLYSMIC VARIABLES; PRIMARY STARS; RADIAL VELOCITY; SECONDARY STARS; STAR: INDIVIDUAL: BT MON; STARS: INDIVIDUAL: PROXIMA CENTAURI; WEAK ABSORPTION;

WHITE DWARFS;

EID: 0001670480     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1998.00743.x     Document Type: Article

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