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NLTE Synthetic Spectra of Mira-Type Variable Stars

Published online by Cambridge University Press:  15 February 2018

Donald G. Luttermoser ,
George H. Bowen  and
Lee Anne Willson
Donald G. Luttermoser
Affiliation:
Iowa State University, Ames, Iowa, USA
George H. Bowen
Affiliation:
Iowa State University, Ames, Iowa, USA
Lee Anne Willson
Affiliation:
Iowa State University, Ames, Iowa, USA

Abstract

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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.

Type
Beyond the Classical Instability Strip
Information
International Astronomical Union Colloquium , Volume 139: New Perspectives on Stellar Pulsation and Pulsating Variable Stars , 1993 , pp. 207
Copyright
Copyright © Cambridge University Press 1993

References

Bowen, G.H. 1988, ApJ, 339, 299.CrossRefGoogle Scholar
Brugel, E.W., Beach, T.E., Willson, L.A., & Bowen, G.H. 1988, in IAU Coll. #103, The Symbiotic Phenomenon, 67.CrossRefGoogle Scholar
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.Google Scholar