A 6.3-h superhump in the cataclysmic variable TV Columbae: The longest yet seen

Monthly Notices of the Royal Astronomical Society

Volumn 340, Issue 2, 2003, Pages 679-686

  Retter, A ^a,b   Hellier, C ^b   Augusteijn, T ^c   Naylor, T ^b,d   Bedding, T R ^a   Bembrick, C ^e   McCormick, J ^f   Velthuis, F ^f  

^a UNIVERSITY OF SYDNEY   (Australia)

^b KEELE UNIVERSITY   (United Kingdom)

^c NORDIC OPTICAL TELESCOPE   (Spain)

^d UNIVERSITY OF EXETER   (United Kingdom)

^e Mt Tarana Observatory   (Australia)

^f Farm Cove Observatory   (New Zealand)

Author keywords

Accretion, accretion discs; Novae, cataclysmic variables; Stars: individual: TV Col

Indexed keywords

ACCRETION: ACCRETION DISKS; CATACLYSMIC VARIABLES; CURRENT THEORIES; MASS RATIO; NOVAE CATACLYSMIC VARIABLES; ORBITAL PERIODS; PHOTOMETRIC DATA; PHOTOMETRICS; STAR: INDIVIDUAL: TV COL; STARS: INDIVIDUAL: PROXIMA CENTAURI;

PHOTOMETRY;

EID: 0043120250     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06331.x     Document Type: Article

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