Helium runaways in white dwarfs

Details Helium runaways in white dwarfs Helium runaways in white dwarfs

Aug 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979stin...8016986t&link_type=abstract

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Physics

Helium, Novae, Stellar Evolution, Stellar Mass Accretion, White Dwarf Stars, Carbon, Gas Temperature, Graphs (Charts), High Temperature Gases, Tables (Data), Thermonuclear Reactions

Scientific paper

The long term evolution of an accreting carbon white dwarf was studied from the onset of accretion to the ignition of helium. The variations in the details of the helium shell flash examined with respect to variations in mass accretion rate. For intermediate rates the helium flash is potentially explosive whereas for high rates the shell flash is relatively weak. The results are discussed in the context of the long term evolution of novae.

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