The AMIGA sample of isolated galaxies. VII. Far-infrared and radio continuum study of nuclear activity

Abstract

We present a study of the nuclear activity in a well-defined sample of the most isolated galaxies in the local Universe traced by their far-infrared (FIR) and radio continuum emission. We use the well-known radio continuum-FIR correlation to select radio-excess galaxies that are candidates to host an active galactic nucleus (AGN), as well as the FIR colours to find obscured AGN candidates. The existing information on nuclear activity in the Véron-Cetty catalogue and in the NASA Extragalactic Database are also used. A final catalogue of AGN-candidate galaxies has been produced. It contains 89 AGN candidates and is publicly available on the AMIGA web page (http://www.iaa.csic.es/AMIGA.html). At most ~ 1.5 % of the galaxies shows a radio-excess with respect to the radio-FIR correlation, and this fraction even goes down to less than 0.8 % after rejection of back/foreground sources. We find that the fraction of FIR colour selected AGN-candidates is ~ 28 % with a lower limit of ~ 7 %. A comparison with the results from the literature shows that the AMIGA sample has the lowest ratio of AGN candidates, both globally and separated into early and late types. Field galaxies as well as poor cluster and group environments show intermediate values, while the highest rates of AGN candidates are found in the central parts of clusters and in pair/merger dominated samples. We conclude that the environment plays a crucial and direct role in triggering radio nuclear activity and not only via the density-morphology relation. Isolated, early-type galaxies show a particularly low level of activity at radio wavelengths hence constituting the most nurture-free population of luminous early-type galaxies.