Disk-instability model for outbursts of dwarf novae - Fine mesh calculations

Details Disk-instability model for outbursts of dwarf novae - Fine mesh calculations Disk-instability model for outbursts of dwarf novae - Fine mesh calculations

Feb 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.130..331m&link_type=abstract

(IAU, DFG, and Bayerisches Staatsministerium für Unterricht und Kultus, Colloquium on Cataclysmic Variables, Recent Multi-Freque

Statistics

Computation

17

Accretion Disks, Computational Grids, Dwarf Novae, Stellar Mass Ejection, Stellar Models, Stellar Temperature, Thermal Diffusion

Scientific paper

The author has executed fine mesh calculations which can almost fully resolve the transition front in the accretion disk of dwarf novae. Results show that the effects of thermal diffusion become very important only when the heating wave passes by, but it is unlikely that they cause drastic changes in the situation of wave propagation. The validity of the localized front approximation is examined. It is found that this approximation is relatively good for heating waves but it is marginal for cooling waves.

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