- Abstract:
-
We used the CLUMPY torus models and a Bayesian approach to fit the infrared spectral energy distributions and ground-based high angular resolution mid-infrared spectroscopy of 13 nearby Seyfert galaxies. This allowed us to put tight constraints on torus model parameters such as the viewing angle i, the radial thickness of the torus Y, the angular size of the cloud distribution σtorus, and the average number of clouds along radial equatorial rays N0. We found that the viewing angle i is not th...
Expand abstract - Publication status:
- Published
- Publisher copy:
- 10.1088/0004-637X/736/2/82
-
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- Publisher:
- Institute of Physics Publishing
- Journal:
- ASTROPHYSICAL JOURNAL
- Volume:
- 736
- Issue:
- 2
- Pages:
- 82-82
- Publication date:
- 2011-08-01
- DOI:
- EISSN:
-
1538-4357
- ISSN:
-
0004-637X
- URN:
-
uuid:8651be19-d80d-4775-ad3b-f65bc0af7269
- Source identifiers:
-
172176
- Local pid:
- pubs:172176
- Language:
- English
- Keywords:
- Copyright date:
- 2011
Journal article
TORUS AND ACTIVE GALACTIC NUCLEUS PROPERTIES OF NEARBY SEYFERT GALAXIES: RESULTS FROM FITTING INFRARED SPECTRAL ENERGY DISTRIBUTIONS AND SPECTROSCOPY
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