V795 Her: An SW Sex star in the period gap?

Monthly Notices of the Royal Astronomical Society

Volumn 278, Issue 1, 1996, Pages 219-235

  Casares, J ^a   Martinez Pais I G ^b   Marsh, T R ^c   Charles, P A ^a   Lazaro C ^b  

^a UNIVERSITY OF OXFORD   (United Kingdom)

^b INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^c UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

Author keywords

Accretion, accretion discs; Binaries: close; Binaries: spectroscopic; Novae, cataclysmic variables; Stars: individual: V795 Her

Indexed keywords

MODULATION; PHOTOMETRY; SHEAR WAVES; WHITE DWARFS;

ABSORPTION FEATURES; ACCRETION: ACCRETION DISKS; BINARIES: CLOSE; BINARIES: SPECTROSCOPIC; EMISSION LINES; NOVAE CATACLYSMIC VARIABLES; ORBITAL PERIODS; S-WAVES; STAR: INDIVIDUAL: V795 HER; STARS: INDIVIDUAL: PROXIMA CENTAURI;

ELECTROMAGNETIC WAVE EMISSION;

EID: 0000524557     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/278.1.219     Document Type: Article

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