The Mass Distribution of White Dwarfs: An Unwavering Obsession
P. Bergeron, A. Gianninas, S. Boudreault
Abstract
We discuss some of our current knowledge of the mass distribution of DA and non-DA stars using various methods for measuring white dwarf masses including spectroscopic, trigonometric parallax, and gravitational redshift measurements, with a particular emphasis on the problems encountered at the low end of the cooling sequence where energy transport by convection becomes important.
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