The Formation of Hydrogen-Deficient Stars in Binaries

Details The Formation of Hydrogen-Deficient Stars in Binaries The Formation of Hydrogen-Deficient Stars in Binaries

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..391..323p&link_type=abstract

Hydrogen-Deficient Stars ASP Conference Series, Vol. 391, proceedings of the conference held 17-21 September, 2007, at Eberhard

Astronomy and Astrophysics

Astronomy

2

Scientific paper

Binary evolution produces a large number of formation channels for hydrogen-deficient stars. Here I review the main binary interactions, stable and unstable mass transfer, binary mergers, and apply them to a variety of objects, including hot subdwarfs, He-rich sdO stars, AM CVn stars, Type Ia supernova progenitors, ultracool white dwarfs and Type Ic and gamma-ray burst progenitors.

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