Properties of discontinuous and nova-amplified mass transfer in cataclysmic variables

Monthly Notices of the Royal Astronomical Society

Volumn 297, Issue 2, 1998, Pages 633-647

  Schenker, K ^a,c   Kolb, U ^b,c   Ritter, H ^c  

^a UNIVERSITY OF BASEL   (Switzerland)

^b UNIVERSITY OF LEICESTER   (United Kingdom)

^c MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

Author keywords

Binaries: close; Novae, cataclysmic variables; Stars: evolution

Indexed keywords

ANGULAR MOMENTUM; LONG TERM EVOLUTION (LTE); WHITE DWARFS;

ANGULAR MOMENTUM LOSS; BINARIES: CLOSE; CATACLYSMIC VARIABLES; EXPANSION VELOCITY; LONG-TERM EVOLUTION; MASS LOSS; MASS TRANSFER RATE; NOVAE CATACLYSMIC VARIABLES; PROPERTY; STAR: EVOLUTION;

MASS TRANSFER;

EID: 0001241468     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1998.01529.x     Document Type: Article

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