Multifrequency observations of dwarf novae outbursts

Details Multifrequency observations of dwarf novae outbursts Multifrequency observations of dwarf novae outbursts

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985esasp.236...39s&link_type=abstract

In ESA Recent Results on Cataclysmic Variables p 39-45 (SEE N86-20287 10-93)

Astronomy and Astrophysics

Astronomy

10

Cataclysmic Variables, Dwarf Novae, Exosat Satellite, Stellar Activity, Stellar Mass Accretion, Stellar Spectra, Infrared Astronomy, Iue, Polarimetry, Stellar Spectrophotometry

Scientific paper

Studies using EXOSAT and IUE data combined with ground-based optical and IR photometry, spectroscopy and polarimetry of the transition timescales and physical properties of the high accretion rate states of the disks in cataclysmic variables are discussed. Implications for dwarf novae stem from comparison of the timing and amplitude of the optical and IR rise with that of the UV and X-ray; the development of the optical and UV line profile changes as the outburst develops; and the similarity of the outburst flux distributions in different systems and different types of outbursts (standstills and supermaxima). These features of dwarf novae outbursts present interesting comparisons with the outbursts of systems like TV Col and GK Per.

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