The component masses of the cataclysmic variable V347 Puppis

Monthly Notices of the Royal Astronomical Society

Volumn 357, Issue 3, 2005, Pages 881-894

  Thoroughgood, T D ^a   Dhillon, V S ^a   Steeghs, D ^b   Watson, C A ^a   Buckley, D A H ^c   Littlefair, S P ^d   Smith, D A ^a,e   Still, M ^f,h   Van Der Heyden, K J ^c   Warner, B ^g  

^a UNIVERSITY OF SHEFFIELD   (United Kingdom)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^c SOUTH AFRICAN ASTRONOMICAL OBSERVATORY   (South Africa)

^d UNIVERSITY OF EXETER   (United Kingdom)

^e Winchester College   (United Kingdom)

^f NASA GODDARD SPACE FLIGHT CENTER   (United States)

^g UNIVERSITY OF CAPE TOWN   (South Africa)

^h UNIVERSITIES SPACE RESEARCH ASSOCIATION   (United States)

Author keywords

Accretion, accretion discs; Binaries: eclipsing; Binaries: spectroscopic; Novae, cataclysmic variables; Stars: individual: V347 Pup

Indexed keywords

LASER SPECTROSCOPY; VELOCITY; WHITE DWARFS;

ACCRETION: ACCRETION DISKS; BINARIES: SPECTROSCOPIC; BINARIES:ECLIPSING; CATACLYSMIC VARIABLES; NOVAE CATACLYSMIC VARIABLES; RADIAL VELOCITY; SECONDARY STARS; STAR: INDIVIDUAL: V347 PUP; STARS: INDIVIDUAL: PROXIMA CENTAURI; TIME-RESOLVED SPECTROSCOPY;

SHEAR WAVES;

EID: 14544275446     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.08613.x     Document Type: Article

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