DW Cancri: A magnetic VY Scl star with an orbital period of 86 min

Monthly Notices of the Royal Astronomical Society

Volumn 349, Issue 1, 2004, Pages 367-374

  Rodriguez Gil P ^a   Gansicke B T ^a   Araujo Betancor, S ^a   Casares, J ^b  

^a UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

^b INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

Author keywords

Accretion, accretion discs; Binaries: close; Novae, cataclysmic variables; Stars: individual: DW Cnc

Indexed keywords

MASS TRANSFER; SHEAR WAVES; SPECTROSCOPIC ANALYSIS; WHITE DWARFS;

ACCRETION: ACCRETION DISKS; BINARIES: CLOSE; CATACLYSMIC VARIABLES; INTERMEDIATE POLARS; NOVAE CATACLYSMIC VARIABLES; ORBITAL PERIODS; SHORT PERIODS; STAR: INDIVIDUAL: DW CNC; STARS: INDIVIDUAL: PROXIMA CENTAURI; TIME-RESOLVED SPECTROSCOPIC STUDIES;

PHOTOMETRY;

EID: 1842483883     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.07512.x     Document Type: Article

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