Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995stin...9611451m&link_type=abstract
Presented at the 1995 International Astronomical Union (IAU) Colloquium No. 152 on Astrophysics in the Extreme Ultraviolet, Berk
Astronomy and Astrophysics
Astrophysics
Accretion Disks, Cygnus Constellation, Emission Spectra, Extreme Ultraviolet Radiation, Novae, Optical Measurement, Power Spectra, Satellite Observation, Stellar Oscillations, White Dwarf Stars, Extreme Ultraviolet Explorer Satellite, Light (Visible Radiation), Photometry, Stellar Luminosity
Scientific paper
The authors present EUVE Deep Survey photometry and AAVSO optical measurements of the 1993 August and 1994 June/July outbursts of the dwarf nova SS Cygni. The EUV and optical light curves are used to illustrate the different response of the accretion disk to outbursts which begin at the inner edge and propagate outward, and those which begin at the outer edge and propagate inward. Furthermore, the authors describe the properties of the quasi-coherent 7-9 s sinusoidal oscillations in the EUV flux detected during the rise and plateau stages of these outbursts.
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