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Infrared spectra of C-type variables with ISO
Published online by Cambridge University Press: 25 May 2016
Abstract
We present ISO-SWS spectra for several representative AGB carbon stars obtained at several phases of the pulsational cycle. For stars with significant mass loss we correct the spectra for the dust emission by using DUSTY models. We then compare these corrected data to synthetic spectra based on hydrostatic and dynamical model atmospheres. We also discuss the influence of the fundamental model parameters on the resulting synthetic spectra.
- Type
- Part 2. Pulsation, Mass Loss, Cool Envelopes
- Information
- Symposium - International Astronomical Union , Volume 191: Asymptotic Giant Branch Stars , 1999 , pp. 181 - 186
- Copyright
- Copyright © Astronomical Society of the Pacific 1999
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