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 re-
port new results obtained from spectroscopic observations of both members of several CPMPs
composed of a F, G or K type star and a DA white dwarf.
CitationCatalán, S.; Ribas, I.; Isern i Vilaboy, J.; García-Berro, E.; Allende Prieto, C. The initial–final mass relationship of white dwarfs in common proper motion pairs and open clusters. Proceedings of the International Astronomical Union: Symposium 240. 2007, Vol. 2, p. 380-382
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