Disk models for cataclysmic variables

Details Disk models for cataclysmic variables Disk models for cataclysmic variables

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..88..293v&link_type=abstract

Astrophysics and Space Science, vol. 88, no. 2, Dec. 1982, p. 293-297.

Astronomy and Astrophysics

Astrophysics

Convection, Stellar Mass Accretion, Stellar Models, Stellar Structure, Variable Stars, Stellar Luminosity

Scientific paper

This paper presents disk models for cataclysmic variables in which convection in the central layers has been included. The calculation of the vertical structure at different points is presented. The models have a central mass of 1 solar mass and matter fluxes of 10 to the -9th, 10 to the -8th, and 10 to the -7th solar mass/yr. The corresponding luminosities are 1.86, 1.86 x 10 and 1.86 x 10-squared solar luminosities.

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