- Abstract:
-
We present high-resolution mid-infrared (MIR) imaging, nuclear spectral energy distributions (SEDs), and archival Spitzer spectra for 22 low-luminosity active galactic nuclei (LLAGNs; L bol ≲ 10 42 erg s -1). Infrared (IR) observations may advance our understanding of the accretion flows in LLAGNs, the fate of the obscuring torus at low accretion rates, and, perhaps, the star formation histories of these objects. However, while comprehensively studied in higher-luminosity Seyferts and quasars...
Expand abstract - Publication status:
- Published
- Publisher copy:
- 10.1088/0004-6256/144/1/11
-
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- Journal:
- ASTRONOMICAL JOURNAL
- Volume:
- 144
- Issue:
- 1
- Pages:
- 11-11
- Publication date:
- 2012-07-05
- DOI:
- EISSN:
-
1538-3881
- ISSN:
-
0004-6256
- URN:
-
uuid:93170c12-15ca-4589-9415-00bbb8478e68
- Source identifiers:
-
342636
- Local pid:
- pubs:342636
- Language:
- English
- Keywords:
- Copyright date:
- 2012
Journal article
THE NUCLEAR INFRARED EMISSION OF LOW-LUMINOSITY ACTIVE GALACTIC NUCLEI
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