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Kolb, U. and Willems, B.
(2005).
URL: http://www.aspbooks.org/custom/publications/table_...
Abstract
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.