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Convection in the helium flash

VII. Special Topics

Part of the Lecture Notes in Physics book series (LNP,volume 71)

Abstract

The evolution of a star through the helium flash depends upon uncertain aspects of convection theory. Observations place some constraints on the theory of convection in stellar cores.

Keywords

  • Convective Zone
  • Globular Cluster
  • Supernova Remnant
  • Degenerate Electron
  • Burning Region

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.

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  • DOI: 10.1007/3-540-08532-7_51
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© 1977 Springer-Verlag

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Wickett, A.J. (1977). Convection in the helium flash. In: Spiegel, E.A., Zahn, JP. (eds) Problems of Stellar Convection. Lecture Notes in Physics, vol 71. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-08532-7_51

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  • DOI: https://doi.org/10.1007/3-540-08532-7_51

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-08532-4

  • Online ISBN: 978-3-540-35982-1

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