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Preliminary Results of Improved Model Fits to the Extreme and Far UV Observations of Cataclysmic Variables

Published online by Cambridge University Press:  12 April 2016

T.E. Carone ,
R.S. Polidan  and
R.A. Wade
T.E. Carone
Affiliation:
University of Arizona, Lunar and Planetary Laboratory, Tucson, Arizona, U.S.A.
R.S. Polidan
Affiliation:
University of Arizona, Lunar and Planetary Laboratory, Tucson, Arizona, U.S.A.
R.A. Wade
Affiliation:
Steward Observatory, University of Arizona, Tucson, Arizona, U.S.A.

Abstract

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We present the first results of a study which will attempt to analyze the combined Voyager and IUE observations of cataclysmic variables using steady-state accretion disk models. Initially we use flux ratio diagrams to determine if a combination of models will suffice or if new ingredients are necessary.

Type
III. UV and X-Ray Observations
Information
International Astronomical Union Colloquium , Volume 93: Cataclysmic Variables: Recent Multi-Frequency Observations and Theoretical Developments , 1987 , pp. 239 - 242
Copyright
Copyright © Reidel 1987

References

Carone, T.E., Polidan, R.S. and Wade, R.A., Composite Voyager and IUE Spectra of Three Types of Cataclysmic Variables, in Ninth North American Workshop on Cataclysmic Variables, ed. Szkody, P. (Seattle: University of Washington), p. 11, 1985.Google Scholar
Polidan, R.S., Voyager Observations of Cataclysmic Variables, in Ninth North American Workshop on Cataclysmic Variables, ed. Szkody, P. (Seattle: University of Washington), p. 103, 1985.Google Scholar
Wade, R.A., A.J., 87, 1558, 1982.Google Scholar
Wade, R.A., MNRAS, 208, 381, 1984.Google Scholar
Wesemael, F., Auer, L.H., van Horn, H.M. and Savedoff, M.P., Ap. J. Supp., 43, 159, 1980.Google Scholar