Advertisement

Synergetics pp 80-89 | Cite as

Instabilities in Stellar Evolution

  • R. Kippenhahn
Conference paper
Part of the Springer Series in Synergetics book series (SSSYN, volume 2)

Abstract

In the following I first give a brief review of stellar evolution, and I then pick out situations in which the whole star or a part of it becomes unstable. As it occurs at present the process of star formation in our galaxy appears to be a process by which the system (our galaxy), out of irregular motion forms a very regular pattern and therefore seems to belong to these phenomena which are covered by synergetics.

Keywords

Star Formation Stellar Evolution Hydrostatic Equilibrium Solar Mass Hydrogen Burning 
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.

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

  1. 1.
    N. Baker, R. Kippenhahn: Astrophys.J. 142, 868 (1965)ADSCrossRefGoogle Scholar
  2. 2.
    K. Fricke, R. Kippenhahn: Ann. Rev. Astron. Astrophys. 10, 45 (1972)ADSCrossRefGoogle Scholar
  3. 3.
    F. Hohl: IAU Symp. No. 38, 368 (1970)ADSGoogle Scholar
  4. 4.
    R. Kippenhahn, A. Weigert: Sterne u. Weltraum 3, 173 (1964)Google Scholar
  5. 5.
    R.B. Larson: M.N.R.A.S. 145, 271 (1969)ADSGoogle Scholar
  6. 6.
    C.C.Lin: Lectures in Appl. Math. Vol. 9, ed. J. Ehlers, Am. Hath. Soc., Providence, Rhode Island (1967)Google Scholar
  7. 7.
    D.S. Mathewson, P.C. van der Kruit, W.N. Brouw: Astron. Astrophys. 17, 468 (1972)ADSGoogle Scholar
  8. 8.
    R. Wielen: Mitt. Astron. Ges. 30, 31 (1971)ADSGoogle Scholar

Copyright information

© Springer-Verlag Berlin Heidelberg 1977

Authors and Affiliations

  • R. Kippenhahn

There are no affiliations available

Personalised recommendations