An analytic approach to the secular evolution of cataclysmic variables

Monthly Notices of the Royal Astronomical Society

Volumn 279, Issue 2, 1996, Pages 581-590

  Stehle, R ^a,b   Ritter, H ^a   Kolb, U ^a,c  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b UNIVERSITY OF AMSTERDAM   (Netherlands)

^c University of California at Santa Cruz   (United States)

Author keywords

Novae, cataclysmic variables; Stars: evolution; Stars: mass loss

Indexed keywords

LINEARIZATION; MASS TRANSFER; STARS;

ANALYTIC APPROACH; CATACLYSMIC VARIABLES; INITIAL CONDITIONS; LOW-MASS STARS; MASS LOSS; NOVAE CATACLYSMIC VARIABLES; SECULAR EVOLUTION; STAR: EVOLUTION; STARS: MASS-LOSS; TIME-SCALES;

DIFFERENTIAL EQUATIONS;

EID: 0001543585     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/279.2.581     Document Type: Article

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