Direct Evidence from Spitzer for a low-luminosity AGN at the center of the Elliptical Galaxy NGC 315
arXiv:0711.0051 · doi:10.1086/525018
Abstract
We present the {\it Spitzer} Space Telescope InfraRed Array Camera (IRAC) and Multiband Imaging Photometer (MIPS) observations of the elliptical galaxy NGC 315. After removal of the host galaxy's stellar emission, we detected for the first time an infrared-red nucleus in NGC 315. We measured the spectral energy distribution (SED) for this active nucleus with wavelength range covering from radio to X-ray, and obtained the bolometric luminosity of , corresponding to an extremely low Eddington ratio (L/L) of 4.97 10. Our results confirm that the physical nature of the nucleus of NGC 315 is a low-luminosity AGN, consistent with the recent optical and {\it Chandra} X-ray observations.
4 pages, accepted for publication in ApJ Letters
References in corpus (2)
Cited by in corpus (10)
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- Broadband Modeling of Low Luminosity Active Galactic Nuclei Detected in Gamma Rays
- Searching for Nuclear Obscuration in the Infrared Spectra of Nearby FR I Radio Galaxies
- Hard X-ray view of two -ray detected low-luminosity active galactic nuclei: NGC 315 and NGC 4261