Later Phases of Core Evolution

  • Rudolf Kippenhahn
  • Alfred Weigert
  • Achim Weiss
Chapter
Part of the Astronomy and Astrophysics Library book series (AAL)

Abstract

Stars massive enough to ignite nuclear burning cycles beyond helium burning may go through several cycles of core burning, producing increasingly heavier elements, up to iron, in their centres. This is the subject of this chapter.

Keywords

Massive Star White Dwarf Stellar Mass Convective Core Carbon 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.

References

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Copyright information

© Springer-Verlag Berlin Heidelberg 2012

Authors and Affiliations

  • Rudolf Kippenhahn
    • 1
  • Alfred Weigert
    • 2
  • Achim Weiss
    • 3
  1. 1.GöttingenGermany
  2. 2.Universität HamburgHamburgGermany
  3. 3.Max-Planck-Institut für AstrophysikGarchingGermany

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