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Atmospheric Structure and Mass Loss of O-rich Long Period Variables. A Confrontation of Models with ISO-SWS Observations
Published online by Cambridge University Press: 25 May 2016
Abstract
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We present ISO-SWS observations of cool oxygen-rich AGB variables and compare them to synthetic molecular and dust spectra based on hydrostatic and dynamic model atmospheres.
- Type
- Part 2. Pulsation, Mass Loss, Cool Envelopes
- Information
- Symposium - International Astronomical Union , Volume 191: Asymptotic Giant Branch Stars , 1999 , pp. 169 - 174
- Copyright
- Copyright © Astronomical Society of the Pacific 1999
References
Ivezić, Ž., Nenkova, M., Elitzur, M., 1997, User Manual for DUSTY, Internal Report, University of Kentucky, accessible at
http://www.pa.uky.edu/~moshe/dusty
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