The decay of dwarf nova outbursts

Astronomy and Astrophysics – Astronomy

Scientific paper

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Dwarf Novae, Stellar Mass Ejection, Stellar Spectrophotometry, Accretion Disks, Stellar Mass Accretion, Stellar Models, Ultraviolet Spectra, Visible Spectrum, X Ray Spectra

Scientific paper

Simultaneous observations at different wavelengths of the decay of dwarf-nova outbursts are presented. The data obtained from Exosat monitoring of dwarf-nova VW Hyi during and after optical superoutburst are discussed. Observations by Mason et al. (1978) of dwarf-nova U Gem were studied and compared to the VW Hyi data. UV observations of the decay of a normal outburst in VW Hyi, by Schwarzenberg-Czerny et al. (1984), are presented; a comparison of these observations with other studies is provided. The observations revealed that the decay of dwarf-nova outbursts shows an earlier return to the quiescent level at shorter wavelengths.

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