On the asphericity of nova remnants caused by rotating white dwarf envelopes

Monthly Notices of the Royal Astronomical Society

Volumn 296, Issue 4, 1998, Pages 943-948

  Porter, John M ^a   O'Brien, T J ^a   Bode, Mike F ^a  

^a LIVERPOOL JOHN MOORES UNIVERSITY   (United Kingdom)

Author keywords

Hydrodynamics; Novae, cataclysmic variables; Stars: mass loss; White dwarfs

Indexed keywords

WHITE DWARFS;

ASPHERICITY; BINARY STAR SYSTEM; DOMINANT PROCESS; HYDRODYNAMIC SIMULATION; NOVAE CATACLYSMIC VARIABLES; NUMERICAL HYDRODYNAMICS; STARS: MASS-LOSS; THEORETICAL STUDY;

HYDRODYNAMICS;

EID: 0000717050     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1998.01470.x     Document Type: Article

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