The nature of the IR emission in LLAGN at parsec scales
The vast majority of AGN belong to the low-luminosity class (LLAGN): they exhibit a low radiation effciency (L ≲ 1042 erg s−1; L/Ledd ≲ 10−3) and the absence of the big blue bump in their spectrum, a signature of the accretion disk. The study of LLAGN is a complex task due to the contribution of the...
| Main Authors: | , , , , |
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| Format: | Article |
| Language: | English |
| Published: |
EDP Sciences
2013-12-01
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| Series: | EPJ Web of Conferences |
| Online Access: | http://dx.doi.org/10.1051/epjconf/20136104005 |