Multi-wavelength predictions of the DIM

Details Multi-wavelength predictions of the DIM Multi-wavelength predictions of the DIM

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004rmxac..20..257s&link_type=abstract

Compact Binaries in the Galaxy and Beyond, Proceedings of the conference held 17-22 November, 2003 in La Paz, Baja California Su

Astronomy and Astrophysics

Astronomy

Accretion, Accretion Discs, Instabilities, Novae, Cataclysmic Variables, Stars: Individual (Ss Cygni, Vw Hydri)

Scientific paper

Using the disc instability model (DIM) and a simple but reasonable model
for the X-ray, extreme UV, UV and optical emission we investigate the
multi-wavelength properties of dwarf novae. We discuss the predictions
of the model in the context of the observationally best studied systems,
i.e. SS Cyg and VW Hyi.

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