The heating and cooling of WZ SGE

Details The heating and cooling of WZ SGE The heating and cooling of WZ SGE

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993anips..10...96s&link_type=abstract

Cataclysmic Variables and Related Physics, 2nd Technion Haifa Conference. Edited by O. Regev and Giora Shaviv. Annals of the I

Physics

19

Stellar Mass Accretion, Stellar Temperature, White Dwarf Stars, Angular Momentum, Cooling, Heating, Mathematical Models, Novae

Scientific paper

The observations of WZ Sge provide us with the best test for computational codes trying to calculate the accretion process onto a white dwarf. We find that the accreted material on WZ Sge cannot spread over the whole star at least on a time scale of ten years. Numerical models which include the angular momentum of the accreted material provide the best fit to the observations.

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