The Fate of a WD Accreting H-Rich Material at High Rates

Details The Fate of a WD Accreting H-Rich Material at High Rates The Fate of a WD Accreting H-Rich Material at High Rates

Feb 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012jphcs.337a2051i&link_type=abstract

Journal of Physics: Conference Series, Volume 337, Issue 1, pp. 012051 (2012).

Physics

Scientific paper

We study a white dwarf (WD) accreting solar-composition material at
super-Eddington accretion rates. We find that after many cycles of
hydrogen ignition and burning, several large Helium burning flashes
expel the accreted envelope, leaving no net mass accumulation. This
implies that such a system will not undergo accretion induced collapse.

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