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The Initial–Final Mass Relationship of White Dwarfs in Common Proper Motion Pairs and Open Clusters
Published online by Cambridge University Press: 12 July 2007
Abstract
We have studied white dwarfs in common proper motion pairs (CPMPs) to improve the semi-empirical initial–final mass relationship of white dwarfs. In this contribution, we report new results obtained from spectroscopic observations of both members of several CPMPs composed of an F, G or K type star and a DA white dwarf.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 2 , Symposium S240: Binary Stars as Critical Tools & Tests in Contemporary Astrophysics , August 2006 , pp. 380 - 382
- Copyright
- Copyright © International Astronomical Union 2007