The Detection of Silicate Emission from Quasars at 10 and 18 Microns

June 2005 • 2005ApJ...625L..75H

Authors • Hao, Lei • Spoon, H. W. W. • Sloan, G. C. • Marshall, J. A. • Armus, L. • Tielens, A. G. G. M. • Sargent, B. • van Bemmel, I. M. • Charmandaris, V. • Weedman, D. W. • Houck, J. R.

Abstract • We report the spectroscopic detection of silicate emission at 10 and 18 μm in five PG quasars, the first detection of these two features in galaxies outside the Local Group. This finding is consistent with the unification model for active galactic nuclei (AGNs), which predicts that an AGN torus seen pole-on should show a silicate emission feature in the mid-infrared. The strengths of the detected silicate emission features range from 0.12 to 1.25 times the continuum at 10 μm and from 0.20 to 0.79 times the continuum at 18 μm. The silicate grain temperatures inferred from the ratio of 18 μm to 10 μm silicate features under the assumption of optically thin emission range from 140 to 220 K.

Links

• PREPRINT http://arxiv.org/abs/astro-ph/0504423
• NED https://ned.ipac.caltech.edu/uri/NED::InRefcode/2005ApJ...625L..75H
• ELECTR https://doi.org/10.1086%2F431227
• SIMBAD http://simbad.u-strasbg.fr/simbo.pl?bibcode=2005ApJ...625L..75H
• PDF https://iopscience.iop.org/article/10.1086/431227/pdf
• DATA https://irsa.ipac.caltech.edu/bibdata/2005/H/2005ApJ...625L..75H.html
• SPIRES http://inspirehep.net/search?p=find+eprint+astro-ph/0504423