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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.

References

References.

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Kudritzki, R.-P.: 1979, A&A 52, 11 Google Scholar