Gravitational wave emission by cataclysmic variables: Numerical models of semi-detached binaries

Monthly Notices of the Royal Astronomical Society

Volumn 327, Issue 3, 2001, Pages 888-894

  Rezzolla, Luciano ^a,b   Uryu, Koji ^a,c   Yoshida, Shin'ichirou ^a  

^a SISSA   (Italy)

^b UNIVERSITY OF TRIESTE   (Italy)

^c UNIVERSITY OF WISCONSIN MILWAUKEE   (United States)

Author keywords

Binaries: close; Gravitation; Gravitational waves; Hydrodynamics; Novae, cataclysmic variables; Stars: low mass, brown dwarfs

Indexed keywords

GRAVITATIONAL EFFECTS; NUMERICAL MODELS; RELATIVITY; STARS;

BINARIES: CLOSE; BINARY STAR; CATACLYSMIC VARIABLES; DRIVING FORCES; GRAVITATIONAL-WAVE EMISSION; NOVAE CATACLYSMIC VARIABLES; ROCHE MODELS; SHORT PERIODS; STARS: LOW-MASS BROWN DWARFS; THEORETICAL MINIMUM;

GRAVITY WAVES;

EID: 0041411125     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2001.04796.x     Document Type: Article

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