Detection of superhumps in the VY Scl-type nova-like variable KR Aur

Monthly Notices of the Royal Astronomical Society

Volumn 378, Issue 3, 2007, Pages 955-960

  Kozhevnikov, V P ^a  

^a URAL FEDERAL UNIVERSITY   (Russian Federation)

Author keywords

Novae, cataclysmic variables; Stars: individual: KR Aur; Stars: oscillations

Indexed keywords

ACCRETION DISCS; BRIGHTNESS VARIATIONS; MULTI CHANNEL; NOVAE CATACLYSMIC VARIABLES; NUCLEAR BURNING; SOFT X-RAY; STAR OSCILLATIONS; STAR: INDIVIDUAL: KR AUR; STARS: BE; STARS: INDIVIDUAL: PROXIMA CENTAURI;

WHITE DWARFS;

EID: 34250687389     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.11819.x     Document Type: Article

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