Kolb, U. and Willems, B.
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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.
|Item Type:||Conference Item|
|Extra Information:||ISBN 1583811931|
|Academic Unit/Department:||Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||Christopher Biggs|
|Date Deposited:||20 Dec 2006|
|Last Modified:||02 Aug 2016 13:02|
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