Abstract
This is a progress report on our luminosity function of 329 Palomar Green DA white dwarfs, all reobserved with CCD spectrophotometry and analyzed in the manner of Bergeron, Saffer & Liebert (1992). The combined luminosity and mass functions are presented. Three distinct mass groups of white dwarfs may be identified: (1) the predominant peak group with a median mass just below 0.6 M⊙; (2) the component of likely close binaries where the visible white dwarf is composed of a helium interior and mass < 0.5M⊙; and, (3) massive white dwarfs ≥ 0.9M⊙. This last group includes all three magnetic DA stars for which a measurement or estimate of the mass and radius are available.
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© 1997 Springer Science+Business Media Dordrecht
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Liebert, J., Fleming, T.A., Holberg, J.B., Bergeron, P., Saffer, R.A. (1997). Towards a Luminosity Function of Hot DA White Dwarfs. In: Isern, J., Hernanz, M., García-Berro, E. (eds) White Dwarfs. Astrophysics and Space Science Library, vol 214. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-5542-7_14
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DOI: https://doi.org/10.1007/978-94-011-5542-7_14
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