Thermal-timescale mass transfer and evolved donor stars in CVs

Details Thermal-timescale mass transfer and evolved donor stars in CVs Thermal-timescale mass transfer and evolved donor stars in CVs

Aug 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..330...17k&link_type=abstract

The Astrophysics of Cataclysmic Variables and Related Objects, Proceedings of ASP Conference Vol. 330. Edited by J.-M. Hameury a

Astronomy and Astrophysics

Astrophysics

8

Scientific paper

In the light of mounting evidence that a significant fraction of short-period, angular momentum-driven CVs have a somewhat evolved donor star we present tailor-made population synthesis calculations of newborn CVs and post-common envelope white dwarf binaries. We study the impact of evolutionary parameters on the number of CVs with an evolved donor star. Our models include systems that will undergo a thermal-timescale mass transfer phase.

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