Periodic variabilities in the IUE spectra of SS Cygni

Details Periodic variabilities in the IUE spectra of SS Cygni Periodic variabilities in the IUE spectra of SS Cygni

Feb 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.130..275l&link_type=abstract

(IAU, DFG, and Bayerisches Staatsministerium für Unterricht und Kultus, Colloquium on Cataclysmic Variables, Recent Multi-Freque

Astronomy and Astrophysics

Astrophysics

11

Cataclysmic Variables, Dwarf Novae, Iue, Stellar Orbits, Stellar Spectra, Ultraviolet Spectra, Accretion Disks, White Dwarf Stars

Scientific paper

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 dependent 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.

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