SS Cygni: Accretion disk morphology

Details SS Cygni: Accretion disk morphology SS Cygni: Accretion disk morphology

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.218..391g&link_type=abstract

In ESA 4th European IUE Conf. p 391-393 (SEE N84-35135 24-88)

Astronomy and Astrophysics

Astronomy

5

Accretion Disks, Cygnus Constellation, Stellar Structure, Variable Stars, Balmer Series, Iue, Spaceborne Astronomy, Ultraviolet Spectroscopy, X Ray Sources

Scientific paper

The authors present an extensive study of IUE spectra of SS Cygni in quiescence together with optical medium dispersion spectra. The ultraviolet spectrum shows a power law distribution Fλ∝λα. The values of α best-fitting the spectra, are roughly -4 and -1 shortward and longward ≡1450 Å, respectively. The optical spectra show double peaked Balmer lines occasionally masked by a low velocity emission.

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