How two cohabiting magnetic dynamos explain the secular evolution of cataclysmic variables

Monthly Notices of the Royal Astronomical Society

Volumn 289, Issue 1, 1997, Pages 59-65

  Zangrilli, Luca ^a   Tout, Christopher A ^b,c   Bianchini, Antonio ^a  

^a UNIVERSITY OF PADOVA   (Italy)

^b INSTITUTE OF EXPERIMENTAL MEDICINE   (Hungary)

^c UNIVERSITY OF CAMBRIDGE   (United Kingdom)

Author keywords

Binaries: close; Novae, cataclysmic variables; Stars: evolution; Stars: magnetic fields; Stars: mass loss

Indexed keywords

BOUNDARY LAYERS; GRAVITATION; INTERACTIVE DEVICES; MAGNETISM; MASS TRANSFER; RADIATION EFFECTS;

BINARIES: CLOSE; CATACLYSMIC VARIABLES; CONVECTIVE ENVELOPE; MAGNETIC DYNAMOS; MASS TRANSFER RATE; NOVAE CATACLYSMIC VARIABLES; SECULAR EVOLUTION; STAR: EVOLUTION; STARS: MAGNETIC FIELD; STARS: MASS-LOSS;

STARS;

EID: 0039282658     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/289.1.59     Document Type: Article

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