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Two-Fluid Calculations with Conduction of X-Ray Emission from Accreting Nonmagnetic Degenerate Dwarfs

Published online by Cambridge University Press:  12 April 2016

J. N. Imamura ,
R. H. Durisen ,
D. Q. Lamb  and
G. J. Weast
J. N. Imamura
Affiliation:
Department of Astronomy, Indiana University
R. H. Durisen
Affiliation:
Department of Astronomy, Indiana University
D. Q. Lamb
Affiliation:
Department of Physics, Massachusetts Institute of Technology Department of Physics, University of Illinois
G. J. Weast
Affiliation:
Department of Physics, Massachusetts Institute of Technology Department of Physics, University of Illinois

Extract

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Kylafis and Lamb (1979, hereafter KL) have recently completed a comprehensive study of X-ray emission from accreting nonmagnetic degenerate dwarfs. Their calculations assumed a common temperature for the electrons and the ions, and neglected electron conduction. However, when Compton cooling of the X-ray emission region becomes important at high masses, electron conduction begins to play a role (Kylafis 1978).

Type
Colloquium Session VI
Information
International Astronomical Union Colloquium , Volume 53: White Dwarfs and Variable Degenerate Stars , August 1979 , pp. 406 - 411
Copyright
Copyright © The University of Rochester 1979

References

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