THE NUCLEAR INFRARED EMISSION OF LOW-LUMINOSITY ACTIVE GALACTIC NUCLEI

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 sub(bol) 10 super(42) erg s super(-1)). Infrared (IR) observations may advance our understanding of the accretion...

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Veröffentlicht in:	The Astronomical journal 2012-07, Vol.144 (1), p.1-27
Hauptverfasser:	Mason, R E, Lopez-Rodriguez, E, Packham, C, Alonso-Herrero, A, Levenson, N A, Radomski, J, Almeida, C Ramos, Colina, L, Elitzur, M, ARETXAGA, I, Roche, P F, OI, N
Format:	Artikel
Sprache:	eng
Schlagworte:	ACCRETION DISKS Active galactic nuclei ASTROPHYSICS, COSMOLOGY AND ASTRONOMY Categories COMPUTERIZED SIMULATION COSMIC DUST Density Dust Emission ENERGY SPECTRA GALAXY NUCLEI HYDROGEN Infrared Infrared radiation JETS LUMINOSITY Mathematical models PHOTOMETRY PHOTON EMISSION POLYCYCLIC AROMATIC HYDROCARBONS QUASARS RESOLUTION SEYFERT GALAXIES SILICATES STARS SYNCHROTRON RADIATION
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