AE aquarii: How cataclysmic variables descend from supersoft binaries

Monthly Notices of the Royal Astronomical Society

Volumn 337, Issue 3, 2002, Pages 1105-1112

  Schenker, K ^a   King, A R ^a   Kolb, U ^b   Wynn, G A ^a   Zhang, Z ^a,b,c  

^a UNIVERSITY OF LEICESTER   (United Kingdom)

^b OPEN UNIVERSITY   (United Kingdom)

^c CHINESE ACADEMY OF SCIENCES   (China)

Author keywords

Binaries: close; Cataclysmic variables; Novae; Stars: abundances; Stars: evolution; Stars: individual: AE Aqr; Stars: individual: AM CVn

Indexed keywords

ULTRAVIOLET SPECTROSCOPY;

BINARIES: CLOSE; CATACLYSMIC VARIABLES; NOVA; STAR: EVOLUTION; STAR: INDIVIDUAL: AE AQUARII; STAR: INDIVIDUAL: AM CVN; STARS ABUNDANCES; STARS: INDIVIDUAL: PROXIMA CENTAURI; TIME-SCALES;

STARS;

EID: 0012909978     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2002.05999.x     Document Type: Article

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