Gas flow in cataclysmic variable stars

Details Gas flow in cataclysmic variable stars Gas flow in cataclysmic variable stars

Nov 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...201..661f&link_type=abstract

Astrophysical Journal, vol. 201, Nov. 1, 1975, pt. 1, p. 661-694.

Astronomy and Astrophysics

Astrophysics

33

Binary Stars, Dwarf Stars, Gas Flow, Novae, Variable Stars, Astronomical Models, Hydrodynamics, Mass Transfer, Radiant Cooling, Shock Wave Propagation, Stellar Gravitation, Stellar Mass Ejection

Scientific paper

A description is given of a general method for simulating gas flow in
binary stars. The method is employed to examine mass transfer in a
system resembling the short-period cataclysmic variable stars including
novae, recurrent novae, dwarf novae, and nova-like variables. The system
investigated is scaled to resemble the dwarf nova Z Cam.

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