The Vertical Structure of Accretion Disks for Dwarf Novae

Details The Vertical Structure of Accretion Disks for Dwarf Novae The Vertical Structure of Accretion Disks for Dwarf Novae

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985jass....2....7c&link_type=abstract

Journal of Astronomy and Space Science, vol. 2, no. 1, p. 7-18.

Astronomy and Astrophysics

Astronomy

Scientific paper

We have constructed models of steady state accretion disk with accretion
rate M=1016g/sec or 1018g/sec. The mass and the
radius of white dwarf were taken as 1 Msolar and
109cm, respectively. The possible application of the results
to Z Cha and ZCam are discussed.

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