Hostname: page-component-84b7d79bbc-5lx2p Total loading time: 0 Render date: 2024-07-26T17:37:28.355Z Has data issue: false hasContentIssue false
  • English
  • Français

Hydrogen and Helium Burning in the Degenerate Envelopes of C–O Dwarfs

Published online by Cambridge University Press:  12 April 2016

E.V. Ergma  and
A.V. Tutukov
E.V. Ergma
Affiliation:
Astronomical Council, USSR Academy of Sciences
A.V. Tutukov
Affiliation:
Astronomical Council, USSR Academy of Sciences

Extract

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.

In our previous papers (Tutukov, Ergma, 1979; Ergma and Tutukov, 1979) we have proposed a simple analytical method to investigate the thermal evolution of shells accreted onto the surface of a neutron star. We have used this method for investigation of thermal evolution of shells accreted onto the surface of a carbon-oxygen white dwarf.

Type
Colloquium Session IV
Information
International Astronomical Union Colloquium , Volume 53: White Dwarfs and Variable Degenerate Stars , August 1979 , pp. 269 - 273
Copyright
Copyright © The University of Rochester 1979

References

Chechetkin, V.M., Gershtein, S.S., Imshennik, V.S., Ivanova, L.N., Khlopov, M.Yu. 1979, Preprint IHEP, 78–158.Google Scholar
Ergma, E.V., Tutukov, A.V. 1976, Acta Astron., 26, 69.Google Scholar
Ergma, E.V., Tutukov, A.V. 1979, Astron. Astrophys., (In press).Google Scholar
Tutukov, A.V., Ergma, E.V. 1979, Pisma Astron. Zhurn., 5, 34.Google Scholar