| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1780318 | New Astronomy Reviews | 2006 | 4 Pages |
Abstract
AGN can be dust-hidden by two ways and this talk considers how to unveil them in the infrared: firstly, the powerful 3CR radio galaxies, i.e., type-2 AGN which suffer from anisotropic obscuration of the nuclear region by the dust torus, and secondly, type-1 quasars, which seem to be isotropically reddened by dust, so that they escape detection via optical-UV colour criteria.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
Martin Haas,