Open AccessThe excess far‐infrared emission of active galactic nuclei in the local Universe
Author(s) -
Pasquali A.,
Kauffmann G.,
Heckman T. M.
Publication year - 2005
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1111/j.1365-2966.2005.09290.x
Subject(s) - physics , astrophysics , active galactic nucleus , galaxy , luminous infrared galaxy , redshift , astronomy , sky , star formation , infrared , stellar population , stars , population , emission spectrum , extragalactic astronomy , spectral line , demography , sociology
We have cross‐correlated the Sloan Digital Sky Survey (SDSS) second data release spectroscopic galaxy sample with the IRAS Faint Source Catalogue (FSC). Optical emission line ratios are used to classify the galaxies with reliable IRAS 60‐ and 100‐μm detections into active galactic nuclei (AGN) and normal star‐forming galaxies. We then create subsamples of normal galaxies and AGN that are very closely matched in terms of key physical properties such as stellar mass, redshift, size, concentration and mean stellar age (as measured by absorption line indicators in the SDSS spectra). We then quantify whether there are systematic differences between the infrared (IR) luminosities of the galaxies and the AGN in the matched subsamples. We find that the AGN exhibit a significant excess in far‐infrared (FIR) emission relative to the star‐forming galaxies in our sample. The excesses at 60 and 100 μm are 0.21 ± 0.03 and 0.12 ± 0.035 dex in log L 60 / M ★ and log L 100 / M ★ , respectively. We then discuss whether the FIR excess is produced by radiation from the active nucleus that is absorbed by dust or, alternatively, by an extra population of young stars that is not detectable at optical wavelengths.