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Infrared Radiation from Evolved Stars

Published online by Cambridge University Press:  08 February 2017

William K. Rose
William K. Rose*
Affiliation:
Astronomy Program University of Maryland College Park, MD 20742 USA

Abstract

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OH/IR stars and carbon stars are examples of evolved stars known to lose mass rapidly. In a recent paper (Rose 1987) we have described calculations of infrared continuum radiation from dust in stellar winds from red giants. We compare calculated radiative models with recent infrared measurements and estimate the total contribution of evolved stars to the mid-infrared background radiation observed from the Milky Way and M31.

Type
II. Galactic Background Starlight from UV to IR: Observations and Models
Information
Symposium - International Astronomical Union , Volume 139: The Galactic and Extragalactic Background Radiation , 1990 , pp. 118 - 120
Copyright
Copyright © Kluwer 1990 

References

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