Anisotropy in the mid-IR emission of Seyfert galaxies

Bibcode
2001qhte.conf..255P
Pérez Garcia, A. M.; Rodriguez Espinosa, J. M.
Bibliographical reference

QSO hosts and their environments, Proceedings of an international workshop, held January 10-12, 2001, in Granada, Spain Edited by Isabel Márquez, Josefa Masegosa, Ascencion Del Olmo, Lucas Lara, Emilio García, and Josefina Molina. Dordrecht: Kluwer Academic / Plenum Publishers, 2001 xvii, 376 p. ISBN 0306466627, p.255

Advertised on:
0
2001
Number of authors
2
IAC number of authors
0
Citations
0
Refereed citations
0
Description
Based on Mid and far-IR data of a complete set of Seyfert galaxies we analyse the Spectral Energy Distributions (SED) of these objects. These SEDs can be separated into three thermal emission components. This separation can be used to introduce some sort of spatial resolution in the inherently low resolution ISO data. It can also be applied as a method for detecting galactic disc components in high-z objects. The separation into emission components allows the study of these independently. In particular differences in the emission of the type 1 and 2 Seyferts can be seen in the warm emission component supposedly originated in dust heated by the nuclear source. The colder components tell us about the extended host galaxies.
Type
Non-refereed

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