The rapid evolution of the born-again giant Sakurai ’ s object

@inproceedings{Asplund1998TheRE,
  title={The rapid evolution of the born-again giant Sakurai ’ s object},
  author={M. S. Fredrik Asplund and David L. Lambert and T. Kipper and Don L. Pollacco and M. D. Shetrone},
  year={1998}
}
The extraordinarily rapid evolution of the born-again giant Sakurai’s object following discovery in 1996 has been investigated. The evolution can be traced both in a continued cooling of the stellar surface and dramatic changes in chemical composition on a timescale of a mere few months. The abundance alterations are the results of the mixing and nuclear reactions which have ensued due to the final He-shell flash which occurred during the descent along the white dwarf cooling track. The… CONTINUE READING

References

Publications referenced by this paper.

A&A 294, 453 This article was processed by the author using Springer-Verlag LTEX A&A style file L-AA version

Schenectady, in press van Genderen A.M, A Gautschy
1995

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