Physical Models of White Dwarf Spectral Evolution

Details Physical Models of White Dwarf Spectral Evolution Physical Models of White Dwarf Spectral Evolution

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aas...208.7403c&link_type=abstract

American Astronomical Society, AAS Meeting #208, #74.03

Astronomy and Astrophysics

Astronomy

Scientific paper

We present a white dwarf spectral evolution model featuring a realistic treatment of Hydrogen-Helium mixing and a self-consistent boundary condition. A parameter study on initial mass of hydrogen layer and ISM accretion rate is done with the intention of explaining the observed correlations between white dwarf effective temperature and spectral type. e.g. Bergeron, Ruiz and Leggett (1997).

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