Carbon and oxygen enrichment of the white dwarf outer layer

Statistics – Computation

Scientific paper

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B Stars, Binary Stars, Carbon Stars, Oxygen, White Dwarf Stars, Helium, Stellar Mass Accretion, Stellar Structure

Scientific paper

The paper studies the evolution of matter accreting on a helium dwarf in
a binary system. The computations indicate that the accretion process
may lead to the enrichment of the white dwarf outer layer with carbon
and oxygen. Subsequent accretion on the white dwarf with a carbon- and
oxygen-enriched outer layer may result in a nova phenomenon.

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