Outer boundary conditions for evolving cool WD (original) (raw)

2012

Abstract

ABSTRACT Outer boundary conditions (temperature, pressure, outer stellar mass and geometrical depth) at a Rosseland mean optical depth 25.1189, for effective temperatures between 2000K and 40000K, and 5.5<logg<9.0. These calculations, based on detailed stellar atmosphere models, are appropriated for computing the evolution of cool white dwarfs with hydrogen envelopes. (1 data file).

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