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NLTE Synthetic Spectra of Mira-Type Variable Stars

  • Donald G. Luttermoser (a1), George H. Bowen (a1) and Lee Anne Willson (a1)

Abstract

We present NLTE radiative transfer in hydrodynamic models representative of Mira-type variable stars. Calculations were carried out with the PANDORA code of the Bowen models using a snapshot approximation.

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Copyright

References

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Bowen, G.H. 1988, ApJ, 339, 299.
Brugel, E.W., Beach, T.E., Willson, L.A., & Bowen, G.H. 1988, in IAU Coll. #103, The Symbiotic Phenomenon, 67.
Luttermoser, D.G., & Bowen, G.H. 1992, in Cool Stars, Stellar Systems, and the Sun, eds. Giampapa, M.S. & Bookbinder, J.A. (ASP Conf. Series), 26, 558.

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