The outbursts of dwarf novae

Computer Science

Scientific paper

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Accretion Disks, Dwarf Novae, Stellar Luminosity, Stellar Models, Data Correlation, Steady State, Stellar Atmospheres, Stellar Temperature, Ultraviolet Spectra

Scientific paper

The dwarf nova VW Hydri has been observed simultaneously in the UV and optical at several stages of outburst. An attempt is made to model the spectrum using a steady-state model disc that radiates locally as a Kurucz atmosphere, together with an optically thin component. The spectrum on the rise is inconsistent with a steady disc, and may potentially be used to discriminate between possible outburst mechanisms.

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