, Volume 18, Issue 1, pp 80–85 | Cite as

Convection in degenerate shells of neutron stars

  • V. A. Urpin


Convection Neutron Star 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.


Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

Literature Cited

  1. 1.
    G. Baym, C. J. Pethick, and P. Sutherland, Astrophys. J.,170 299 (1971).Google Scholar
  2. 2.
    J. P. Hansen, Phys. Rev. A8, 3096 (1973).Google Scholar
  3. 3.
    E. L. Pollock and J. P. Hansen, Phys. Rev., A8, 3110 (1973).Google Scholar
  4. 4.
    V. A. Urpin and D. H. Yakovlev, Astrofizika.,15, 647 (1979).Google Scholar
  5. 5.
    D. K. Nadezhin, Nauchn. Informatsii, Astrosovet Akad. Nauk SSSR,32, 3 (1974).Google Scholar
  6. 6.
    S. Chandrasekhar, Hydrodynamic and Hydromagnetic Stability, Oxford (1961).Google Scholar
  7. 7.
    S. I. Braginskii, in: Reviews of Plasma Physics, Vol. 1, Consultants Bureau, New York (1965), p.205.Google Scholar
  8. 8.
    S. Tsuruta and A. G. W. Cameron, Can. J. Phys.,44, 1863 (1966).Google Scholar
  9. 9.
    K. H. Bôhm and J. Cassinelli, Astron. Astrophys.,12, 21 (1971).Google Scholar
  10. 10.
    K. H. Bôhm, Astrophys. Space Sci.,2, 375 (1968).Google Scholar
  11. 11.
    D. G. Yakovlev and V. A. Urpin, Astron. Zh.,57, 526 (1980).Google Scholar
  12. 12.
    R. E. Gershberg, in: Eruptive Stars [in Russian], (eds.,. A. A. Boyarchuk and R. E. Gershberg), Nauka, Moscow (1970).Google Scholar

Copyright information

© Plenum Publishing Corporation 1982

Authors and Affiliations

  • V. A. Urpin

There are no affiliations available

Personalised recommendations