Hostname: page-component-78c5997874-dh8gc Total loading time: 0 Render date: 2024-11-07T22:57:28.606Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

REFERENCES

Bedijn, P. J. 1987, Astron. Astrophys., 186, 136.Google Scholar
Cox, P., Krugel, E., and Mezger, P. G. 1986, Astron. Astrophys., 155, 380.Google Scholar
Knapp, G. R., and Morris, M. 1985, Astrophys. J., 292, 640.Google Scholar
Olnon, F. M., Baud, B., Habing, H. J., DeJong, T., Harris, S., and Pottasch, S. R. 1984, Astrophys. J. (Letters), 278, L41.Google Scholar
Rose, W. K. 1987, Astrophys. J., 312, 284 (Paper I).Google Scholar
Walterbos, R. A. M., and Schwering, P. B. W. 1987, Astron. Astrophys., 180, 27.Google Scholar