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Nuclei of planetary nebulae and white dwarf envelopes

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Abstract

Upper bounds to the masses of He envelopes of white dwarfs are derived by examining the maximum He envelope that a nucleus of a planetary nebulae can have consistent with observation.

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Author notes

  1. A. Kovetz

    Present address: Dept. of Physics and Astronomy, and Dept. of Environmental Sciences, Tel-Aviv Univ., Ramat-Aviv, Israel

Authors and Affiliations

  1. Center for Radiophysics and Space Research, Cornell Univ., Ithaca, N.Y., USA

    G. Shaviv

Authors
  1. A. Kovetz
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  2. G. Shaviv
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Kovetz, A., Shaviv, G. Nuclei of planetary nebulae and white dwarf envelopes. Astrophys Space Sci 23, 385–390 (1973). https://doi.org/10.1007/BF00645165

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  • DOI: https://doi.org/10.1007/BF00645165

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