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WR Central Stars

  • Wolf-Rainer Hamann (a1), Götz Gräfener (a1) and Lars Koesterke (a1)

Abstract

Wolf-Rayet type central stars have been analyzed with adequate model atmospheres. The obtained stellar parameters and chemical abundances allow for a discussion of their evolutionary origin.

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References

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WR Central Stars

  • Wolf-Rainer Hamann (a1), Götz Gräfener (a1) and Lars Koesterke (a1)

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