AMUSE-VIRGO. III: mid-infrared photometry of early-type galaxies and limits on obscured nuclear emission

Details AMUSE-VIRGO. III: mid-infrared photometry of early-type galaxies and limits on obscured nuclear emission AMUSE-VIRGO. III: mid-infrared photometry of early-type galaxies and limits on obscured nuclear emission

2011-11-29

arxiv.org/abs/1111.6774v1

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

17 pages, 8 figures; accepted for publication in ApJ

Scientific paper

We complete our census of low-level nuclear activity in Virgo Cluster early-type galaxies by searching for obscured emission using Spitzer Space Telescope mid-infrared (MIR) imaging at 24mu. Of a total sample of 95 early-type galaxies, 53 objects are detected, including 16 showing kiloparsec-scale dust in optical images. One dimensional and two dimensional surface photometry of the 37 detections without extended dust features reveals that the MIR light is more centrally concentrated than the optical light as traced by Hubble Space Telescope F850LP-band images. No such modeling was performed for the sources with dust detected in the optical images. We explore several possible sources of the MIR excess emission, including obscured nuclear emission. We find that radial metallicity gradients in the stellar population appear to be a natural and most likely explanation for the observed behavior in a majority of the sources. Alternatively, if the concentrated MIR emission were due to nuclear activity, it would imply a MIR-to-X luminosity ratio ~5-10 for the low luminosity AGN detected in X-rays by our survey. This ratio is an order of magnitude larger than that of typical low-luminosity AGN and would imply an unusual spectral energy distribution. We conclude that the black holes found by our survey in quiescent early-type galaxies in Virgo have low bolometric Eddington ratios arising from low accretion rates and/or highly radiatively inefficient accretion.

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