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A 25 micron component in 3C 390.3

Miley, G. and Neugebauer, G. and Soifer, B. T. and Clegg, P. E. and Harris, S. and Rowan-Robinson, M. and Young, E. (1984) A 25 micron component in 3C 390.3. Astrophysical Journal, 278 . L79-L81. ISSN 1538-4357. http://resolver.caltech.edu/CaltechAUTHORS:20170307-140305525

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Abstract

Infrared Astronomical Satellite (IRAS) observations show that there is a maximum in the continuum energy distribution of the broad-line radio galaxy 3C 390.3 near 25µm and that this active galaxy emits most of its energy in the infrared. If the 25µm component is thermal, its temperature is approximately 180 K, and its size must exceed tens of parsecs.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1086/184228DOIArticle
http://adsabs.harvard.edu/abs/1984ApJ...278L..79MADSArticle
Additional Information:© 1984 American Astronomical Society. Received 1983 September 16; accepted 1983 November 18. Without the painstaking efforts of Gene Kopan, Dave Gregorich, Carol Oken, and Linda Fullmer, the reduction of these data would have been impossible.
Subject Keywords:infrared: sources radio sources: galaxies
Record Number:CaltechAUTHORS:20170307-140305525
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20170307-140305525
Official Citation:A 25 micron component in 3C 390.3 Miley, G., Neugebauer, G., Soifer, B. T., Clegg, P. E., Harris, S., Rowan-Robinson, M., , Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 278, March 1, 1984, p. L79-L81.
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:74864
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:07 Mar 2017 22:16
Last Modified:07 Mar 2017 22:16

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