New clues on the nature of the recurrent nova T Coronae Borealis from a light curve of the system spanning 40 years

Monthly Notices of the Royal Astronomical Society

Volumn 287, Issue 3, 1997, Pages 634-640

  Leibowitz, Elia M ^a   Ofek, Eran O ^a   Mattei, Janet A ^b  

^a TEL AVIV UNIVERSITY   (Israel)

^b AMERICAN ASSOCIATION OF VARIABLE STAR OBSERVERS   (United States)

Author keywords

Novae, cataclysmic variables; Stars: individual: T CrB

Indexed keywords

GIANT STARS;

BINARY CYCLES; BOREALIS; D-PERIODICITY; HOT COMPONENTS; LIGHT CURVES; NOVAE CATACLYSMIC VARIABLES; STAR: INDIVIDUAL: T CRB; STARS: INDIVIDUAL: PROXIMA CENTAURI; TIME INTERVAL; VISUAL ESTIMATE;

LUMINANCE;

EID: 0039929175     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/287.3.634     Document Type: Article

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