Hostname: page-component-7479d7b7d-q6k6v Total loading time: 0 Render date: 2024-07-11T06:26:06.320Z Has data issue: false hasContentIssue false

Possible Role of the White Dwarf in Grain Formation in Cataclysmic Variable Systems

Published online by Cambridge University Press:  12 April 2016

J.S. Albinson
Affiliation:
Department of Physics, University of Keele, Keele, Staffordshire, U.K.
A. Evans
Affiliation:
Department of Physics, University of Keele, Keele, Staffordshire, U.K.

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We consider the possibility that carbon, in the form of the allotrope carbyne, might form in the atmosphere of the white dwarf in a cataclysmic variable system, and be expelled from the system by radiation pressure. It seems that, under some circumstances, cataclysmic variable systems may indeed have carbon dust in their vicinity.

Type
V. Nova and Dwarf Nova Outbursts
Copyright
Copyright © Reidel 1987

References

Leiknes, J. & Havnes, O., 1984, Astr. Ap. Suppl., 57, 263 Google Scholar
Pringle, J.E., 1981, Ann. Rev. Astr. Ap., 19, 137 CrossRefGoogle Scholar
Shapiro, S.L. & Teukolsky, S.A., 1983, Black Holes, White Dwarfs and Neutron Stars Wiley, J. & Sons.Google Scholar
Whittaker, A.G., 1978, Science, 200, 763 Google Scholar
Zhilayev, B.E. & Zubko, V.G., 1983, Sov. Astron. Let., 9, 122.Google Scholar
Zhilyaev, B.E. & Zubko, V.G., 1984, Astrophys. Space Sci., 105, 99.CrossRefGoogle Scholar