Publication details for Prof David AlexanderGoulding, A.D., Alexander, D.M., Bauer, F.E., Forman, W.R., Hickox, R.C., Jones, C., Mullaney, J.R. & Trichas, M. (2012). Deep silicate absorption features in Compton-thick active galactic nuclei predominantly arise due to dust in the host galaxy. The astrophysical journal 755(1): 5.
- Publication type: Journal Article
- ISSN/ISBN: 0004-637X (print), 1538-4357 (electronic)
- DOI: 10.1088/0004-637X/755/1/5
- Keywords: Galaxies: active, galaxies: Seyfert, infrared: galaxies, X-rays: galaxies
- Further publication details on publisher web site
- Durham Research Online (DRO) - may include full text
Author(s) from Durham
We explore the origin of mid-infrared (mid-IR) dust extinction in all 20 nearby (z < 0.05) bona fide Compton-thick (N H > 1.5 × 1024 cm-2) active galactic nuclei (AGNs) with hard energy (E > 10 keV) X-ray spectral measurements. We accurately measure the silicate absorption features at λ ~ 9.7 μm in archival low-resolution (R ~ 57-127) Spitzer Infrared Spectrograph spectroscopy, and show that only a minority (≈45%) of nearby Compton-thick AGNs have strong Si-absorption features (S 9.7 = ln (f int/f obs) >~ 0.5) which would indicate significant dust attenuation. The majority (≈60%) are star formation dominated (AGN:SB < 0.5) at mid-IR wavelengths and lack the spectral signatures of AGN activity at optical wavelengths, most likely because the AGN emission lines are optically extinguished. Those Compton-thick AGNs hosted in low-inclination-angle galaxies exhibit a narrow range in Si-absorption (S 9.7 ~ 0-0.3), which is consistent with that predicted by clumpy-torus models. However, on the basis of the IR spectra and additional lines of evidence, we conclude that the dominant contribution to the observed mid-IR dust extinction is dust located in the host galaxy (i.e., due to disturbed morphologies, dust lanes, galaxy inclination angles) and not necessarily a compact obscuring torus surrounding the central engine.