The parsec-scale region of active galactic nuclei in the IR

Bibcode
2004IAUS..222...57P
DOI
10.1017/S1743921304001450
Prieto, M. Almudena; Meisenheimer, Klaus
Bibliographical reference

The Interplay among Black Holes, Stars and ISM in Galactic Nuclei, Proceedings of IAU Symposium, No. 222. Edited by T. Storchi-Bergmann, L.C. Ho, and Henrique R. Schmitt. Cambridge, UK: Cambridge University Press, 2004., p.57-60

Advertised on:
11
2004
Number of authors
2
IAC number of authors
0
Citations
3
Refereed citations
3
Description
First results from the AGN-Heidelberg program aimed at spatially resolving the central pc region of the closest Active Galactic Nuclei are presented. The core region of prototype active nuclei are clearly unveiled at IR waves and at distances from the nucleus - few pc- where circumnuclear starforming regions appear not to be present. Within that perspective, classical active nuclei as Circinus and NGC 1097, reveal with unprecedented detail clear channels of material being driven to the core whereas others as Centaurus A and NGC 5506, show a `clean' core environment. At the very center, a central compact region of ˜2 pc scale is resolved in Circinus but not in the other cases challenging thus the universal presence of the putative obscuring torus.
Type
Non-refereed

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