Abstract

We use Herschel data to analyze the size of the far-infrared 70 mu m emission for z 0.06 local samples of 277 hosts of Swift-BAT selected active galactic nuclei (AGN), and 515 comparison galaxies that are not detected by BAT. For modest far-infrared luminosities 8 : 5 log (L-FIR [L-circle dot]) 10.5, we find large scatter of half light radii R-e,R-70 for both populations, but a typical R-e,R-70 less than or similar to 1 kpc for the BAT hosts that is only half that of comparison galaxies of same far-infrared luminosity. The result mostly reflects a more compact distribution of star formation (and hence gas) in the AGN hosts, but compact AGN heated dust may contribute in some extremely AGN dominated systems. Our findings are in support of an AGN-host coevolution where accretion onto the central black hole and star formation are fed from the same gas reservoir, with more efficient black hole feeding if that reservoir is more concentrated. The significant scatter in the far-infrared sizes emphasizes that we are mostly probing spatial scales much larger than those of actual accretion, and that rapid accretion variations can smear the distinction between the AGN and comparison categories. Large samples are hence needed to detect structural differences that favor feeding of the black hole. No size difference between AGN host and comparison galaxies is observed at higher far-infrared luminosities log(L-FIR [L-circle dot]) > 10.5 (star formation rates greater than or similar to 6 M-circle dot yr(-1)), possibly because these are typically reached in more compact regions.