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The structure and evolution of a slow deflagration front propagating into a degenerate star
Authors:A Braun  R Yahel
Institution:(1) Racah Institute of Physics, Dept. of Theoretical Physics, The Hebrew University of Jerusalem, Israel
Abstract:The structure and evolution of a slow reaction front propagation into a cool, hydrogen rich shell above an inert core has been studied. It has been found that, during the evolution of the front, the total radiative luminosity drops from sim104 L odot to sim10–4 L odot in a time scale of the order of 109 yr. The burned up fraction of the fuel is found to be less than 1%.
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