Emission processes in 3C 270

Details Emission processes in 3C 270 Emission processes in 3C 270

Nov 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004iaus..222...75v&link_type=abstract

The Interplay among Black Holes, Stars and ISM in Galactic Nuclei, Proceedings of IAU Symposium, No. 222. Edited by T. Storchi-B

Physics

1

Scientific paper

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.

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