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Infrared appearance of dynamical models for circumstellar dust shells around long-period variables

  • Session G: AGB Stars, Proto-Planetary Nebulae & Planetary Nebulae
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Abstract

Synthetic brightness profiles resulting from consistent dynamical models for circumstellar dust shells around long-period variables are presented and discussed with respect to a corresponding observation of IRC +10216.

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References

  • Fleischer A. J., Gauger A., Sedlmayr E.: 1992, Astron. & Astrophys.266, 321.

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  • Winters J. M., Dominik C., Sedlmayr E.: 1994a, Astron. & Astrophys.288, 255.

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  • Winters J. M., Fleischer A. J., Gauger A., Sedlmayr, E.: 1994b, Astron. & Astrophys. in press.

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Authors and Affiliations

  1. Institut für Astronomie und Astrophysik, Technische Universität Berlin, Sekr. PN 8-1, Hardenbergstraβe 36, D-10623, Berlin, FRG

    J. M. Winters, A. J. Fleischer & E. Sedlmayr

  2. Los Alamos National Laboratory, Group T-4, MS B268, 87545, Los Alamos, NM, USA

    A. Gauger

Authors
  1. J. M. Winters
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  2. A. J. Fleischer
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  3. E. Sedlmayr
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  4. A. Gauger
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Winters, J.M., Fleischer, A.J., Sedlmayr, E. et al. Infrared appearance of dynamical models for circumstellar dust shells around long-period variables. Astrophys Space Sci 224, 329–332 (1995). https://doi.org/10.1007/BF00667866

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  • DOI: https://doi.org/10.1007/BF00667866

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