Structure of the accretion disk in the dwarf nova Z Cha

Details Structure of the accretion disk in the dwarf nova Z Cha Structure of the accretion disk in the dwarf nova Z Cha

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984azh....61..310d&link_type=abstract

(Astronomicheskii Zhurnal, vol. 61, Mar.-Apr. 1984, p. 310-322) Soviet Astronomy (ISSN 0038-5301), vol. 28, Mar.-Apr. 1984, p. 1

Astronomy and Astrophysics

Astronomy

6

Accretion Disks, Dwarf Novae, Eclipsing Binary Stars, Stellar Structure, Gravitational Waves, Light Curve, Red Dwarf Stars, Stellar Luminosity, White Dwarf Stars

Scientific paper

The eclipse curves of the dwarf nova Z Cha are analyzed in order to determine the structure of the accretion disk of the star in active and inactive states. Brightness temperatures and bolometric luminosities of the accretion disk are given in a table, and the effect of gravitational radiation on the brightness temperatures of the intermediate and peripheral zones of the disk, bolometric luminosity, and the mass loss rate from the red star is discussed in detail.

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