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Spectral analysis and model atmospheres of WR type central stars

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Abstract

Wolf-Rayet type spectra of central stars are compared with spectra from Pop. I objects. Non-LTE models for expanding atmospheres are applied for analyzing these spectra quantitatively.

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Authors and Affiliations

  1. Lehrstuhl Astrophysik der Universität Potsdam, Am Neuen Palais 10, D-14469, Potsdam, Germany

    Wolf-Rainer Hamann

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  1. Wolf-Rainer Hamann
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Hamann, WR. Spectral analysis and model atmospheres of WR type central stars. Astrophys Space Sci 238, 31–42 (1996). https://doi.org/10.1007/BF00645489

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