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On the Computation of Accretion Disk Spectra

Published online by Cambridge University Press:  12 April 2016

C. La Dous
C. La Dous*
Affiliation:
Universitaets-Sternwarte Muenchen, Muenchen, F.R.G.

Abstract

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Spectra of accretion disks in dwarf novae and some novalike stars have been computed. Many simplifications to the general model of the nature of a cataclysmic variable are needed to make the system numerically tractable. The necessity, justification, and implications of such simplifications are discussed together with the influences of some system parameters on the disk radiation.

Type
IV. Accretion Disks
Information
International Astronomical Union Colloquium , Volume 93: Cataclysmic Variables: Recent Multi-Frequency Observations and Theoretical Developments , 1987 , pp. 337 - 340
Copyright
Copyright © Reidel 1987

References

References.

Kudritzki, R.-P.: 1976, 23rd Liege Symp., p. 295 Google Scholar
Kudritzki, R.-P.: 1979, A&A 52, 11 Google Scholar