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Circumstellar Dust Shells

Published online by Cambridge University Press:  14 August 2015

L. M. Shulman
L. M. Shulman*
Affiliation:
The Main Astronomical Observatory of the Ukrainian Academy of Sciences, Kiev

Abstract

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The optical properties of circumstellar graphite particle shells are considered. In the case of the optically thin shell (e.g. the shell of a RCB star after minimum), the temperature of the grains is calculated. It is shown that the dust shell always has a sharp inner border. The RCB phenomenon may be considered as a sudden moving of this border toward the star and the consequent increase in its optical thickness.

Type
Part 2 / R Coronae Borealis Stars
Information
Symposium - International Astronomical Union , Volume 67: Variable Stars and Stellar Evolution , 1975 , pp. 165 - 171
Copyright
Copyright © Reidel 1975 

References

Alexander, J. B., Andrews, P. J., Catchpole, R. M., Feast, M. W., Lloyd Evans, T., Menzies, J. W., Wisse, P. N. J., and Wisse, M.: 1972, Monthly Notices Roy. Astron. Soc. 158, 305.Google Scholar
Feast, M. W. and Glass, I. S.: 1973, Monthly Notices Roy. Astron. Soc. 162, 293.Google Scholar
Herbig, G. H.: 1970, Astrophys. J. 162, 557.Google Scholar
Loreta, E.: 1934, Astron. Nachr. 254, 151.CrossRefGoogle Scholar
Ney, E. P.: 1972, Publ. Astron. Soc. Pacific 84, 613.Google Scholar
O'Keefe, J. A.: 1939, Astrophys. J. 90, 294.Google Scholar
Stein, W. A.: 1972, Publ. Astron. Soc. Pacific 84, 627.Google Scholar