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New Model Sequences from the White Dwarf Evolution Code

Published online by Cambridge University Press:  12 April 2016

M. Wood
M. Wood*
Affiliation:
Department of Physics and Space Sciences, Florida Institute of Technology, Melbourne, FL 32901-6988USA

Abstract

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Model sequences computed with the recently-published OPAL radiative opacities, Itoh et al. conductive opacities, and Itoh et al. neutrino rates are presented. Cooling times for DA model sequences are found to be independent of metallicity for Z ≤ 0.001.

Type
Posters
Information
International Astronomical Union Colloquium , Volume 147: The Equation of State in Astrophysics , 1994 , pp. 612 - 617
Copyright
Copyright © Cambridge University Press 1994

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