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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

B. Aringer ,
F. Kerschbaum ,
J. Hron ,
T. Posch ,
W. Windsteig ,
U.G. Jørgensen  and
S. Höfner
B. Aringer
Affiliation:
Institut für Astronomie, Univ. Wien, Vienna, Austria
F. Kerschbaum
Affiliation:
Institut für Astronomie, Univ. Wien, Vienna, Austria
J. Hron
Affiliation:
Institut für Astronomie, Univ. Wien, Vienna, Austria
T. Posch
Affiliation:
Institut für Astronomie, Univ. Wien, Vienna, Austria
W. Windsteig
Affiliation:
Institut für Astronomie, Univ. Wien, Vienna, Austria
U.G. Jørgensen
Affiliation:
Niels Bohr Institute, Univ. Obs. Copenhagen, Copenhagen, Denmark
S. Höfner
Affiliation:
Niels Bohr Institute, Univ. Obs. Copenhagen, Copenhagen, Denmark

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

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