Evidence for a rotational velocity field about the white dwarf of V347 Puppis

Monthly Notices of the Royal Astronomical Society

Volumn 299, Issue 2, 1998, Pages 545-553

  Still, M D ^a   Buckley, D A H ^b   Garlick, M A ^c  

^a UNIVERSITY OF ST ANDREWS   (United Kingdom)

^b SOUTH AFRICAN ASTRONOMICAL OBSERVATORY   (South Africa)

^c UNIVERSITY OF SUSSEX   (United Kingdom)

Author keywords

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

Indexed keywords

VELOCITY;

ACCRETION: ACCRETION DISKS; BINARIES: SPECTROSCOPIC; BINARIES:ECLIPSING; EXCITATION LINES; LINE: PROFILES; NOVAE CATACLYSMIC VARIABLES; ROTATIONAL VELOCITY; STAR: INDIVIDUAL: V347 PUP; STARS: INDIVIDUAL: PROXIMA CENTAURI; VELOCITY FIELD;

WHITE DWARFS;

EID: 0000153482     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1998.01806.x     Document Type: Article

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