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Radiative Transfer in Nova Envelopes

Published online by Cambridge University Press:  12 April 2016

R.P. Harkness
R.P. Harkness*
Affiliation:
Department of Astrophysics, Oxford University, South Parks Road, Oxford, 0X1 3RQ UK

Extract

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This paper presents some preliminary results of work aimed at producing model atmospheres for the steady-state, constant luminosity continuous ejection model of classical novae. The results are generally, applicable to any object with an outflowing atmosphere driven predominantly by radiation pressure in an optically thick continuum. In particular it is aimed at removing the limitations of assuming blackbody photospheric boundary conditions and strict LTE and the problems associated with their definition.

Type
Colloquium Session VII
Information
International Astronomical Union Colloquium , Volume 53: White Dwarfs and Variable Degenerate Stars , August 1979 , pp. 464 - 468
Copyright
Copyright © The University of Rochester 1979

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