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Emission processes in 3C 270

Published online by Cambridge University Press:  24 November 2004

Ilse M. van Bemmel ,
F. Duccio Macchetto  and
Marco Chiaberge
Ilse M. van Bemmel
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA Space Telescope Division, ESA
F. Duccio Macchetto
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA Space Telescope Division, ESA
Marco Chiaberge
Affiliation:
Istituto de Radioastronomia, Via P.Gobetti 101, I–40129 Bologna, Italy
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Abstract

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We identify the dominant emission processes in 3C 270 in the infrared to be non-thermal, and emission from its dusty disk does not contribute significantly to the total infrared output. This implies that such disks can be hard to find through their infrared emission, and that any circumnuclear torus, if at all present, is small and thin.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
POSTERS
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS222 , March 2004 , pp. 75 - 76
Copyright
© 2004 International Astronomical Union