Superhumps, magnetic fields and the mass ratio in AM Canum Venaticorum

Monthly Notices of the Royal Astronomical Society

Volumn 346, Issue 2, 2003, Pages

  Pearson, K J ^a  

^a LOUISIANA STATE UNIVERSITY   (United States)

Author keywords

Accretion, accretion discs; Binaries: close; Methods: N body simulations; MHD; Novae, cataclysmic variables; Stars: individual: AM CVn

Indexed keywords

ELECTROMAGNETIC FIELD EFFECTS; MAGNETOHYDRODYNAMICS;

ACCRETION: ACCRETION DISKS; BINARIES: CLOSE; MAGNETIC-FIELD; MASS RATIO; METHODS:N-BODY SIMULATIONS; NOVAE CATACLYSMIC VARIABLES; SECONDARY STARS; STAR: INDIVIDUAL: AM CVN; STARS: INDIVIDUAL: PROXIMA CENTAURI; SURFACE STRENGTHS;

STARS;

EID: 0344153841     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-2966.2003.07290.x     Document Type: Article

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