Hostname: page-component-77c89778f8-7drxs Total loading time: 0 Render date: 2024-07-21T06:17:45.828Z Has data issue: false hasContentIssue false
  • English
  • Français

Infrared Emission from Radio Galaxies

Published online by Cambridge University Press:  07 August 2017

C. D. Impey ,
C. G. Wynn-Williams  and
E. E. Becklin
C. D. Impey
Affiliation:
Steward Observatory, University of Arizona, Tucson, Arizona 85721 USA
C. G. Wynn-Williams
Affiliation:
Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, Hawaii 96822 USA
E. E. Becklin
Affiliation:
Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, Hawaii 96822 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.

Observations with the IRTF and IRAS indicate that there are at least two different mechanisms for the generation of infrared emission from radio galaxies.

Type
Part 7: Dust, Molecules, Infrared and MM Radiation
Information
Symposium - International Astronomical Union , Volume 134: Active Galactic Nuclei , 1989 , pp. 404 - 405
Copyright
Copyright © Kluwer 1989 

References

Colla, G., Fanti, C., Fanti, R., Gioia, I., Lari, C., Lequeux, J., Lucas, R., and Ulrich, M. H. 1975, Astr. Ap., 20, 1.Google Scholar
Fanti, C., Fanti, R., de Ruiter, H. R., and Parma, P. 1987, Astr. Ap. Suppl., 69, 57.Google Scholar
Helou, G., Soifer, B. T., and Rowan-Robinson, M. 1985, Ap. J. (Letters), 298, L7.Google Scholar