Astrophysics and Space Science

, Volume 131, Issue 1–2, pp 443–447 | Cite as

Possible role of the white dwarf in grain formation in cataclysmic variable systems

  • J. S. Albinson
  • A. Evans
Nova and Dwarf Nova Outbursts

Abstract

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.

Keywords

Radiation Atmosphere Dust Variable System Radiation Pressure 

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

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

Copyright information

© D. Reidel Publishing Company 1987

Authors and Affiliations

  • J. S. Albinson
    • 1
  • A. Evans
    • 1
  1. 1.Department of PhysicsUniversity of KeeleKeeleUK

Personalised recommendations