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New Model Sequences from the White Dwarf Evolution Code
Published online by Cambridge University Press: 12 April 2016
Abstract
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.
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- International Astronomical Union Colloquium , Volume 147: The Equation of State in Astrophysics , 1994 , pp. 612 - 617
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- Copyright © Cambridge University Press 1994