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Periodic Variabilities in the IUE Spectra of SS Cygni
Published online by Cambridge University Press: 12 April 2016
Abstract
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The analysis of the IUE low resolution spectra of SS Cyg in quiescence clearly shows modulations with the orbital phase of the continuum and the emission lines total area. The shape of such modulations is depending on the type of the optical outburst preceding the quiescent phase in which the UV spectra were collected. This behaviour, together with those in other wavelength regions, could be explained within the framework of the intermediate polar models.
- Type
- III. UV and X-Ray Observations
- Information
- Copyright
- Copyright © Reidel 1987
References
Giovannelli, F., et al.: 1985, in Multifrequency Behaviour of Galactic Accreting Sources, Giovannelli, F. (ed.), Siderea, Roma, P. 37.Google Scholar
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