A&A 436, L5-L8 (2005)
DOI: 10.1051/0004-6361:200500109
Letter
Discovery of 10
m silicate emission in quasars
Evidence of the AGN unification scheme
R. Siebenmorgen1, M. Haas2, E. Krügel3 and B. Schulz41 European Southern Observatory, Karl-Schwarzschildstr. 2, 85748 Garching b. München, Germany
e-mail: rsiebenm@eso.org
2 Astronomisches Institut, Ruhr-Universität, Universitätsstr. 150, 44780 Bochum, Germany
3 Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, Postfach 2024, 53010 Bonn, Germany
4 IPAC, California Institute of Technology (Caltech), Pasadena, CA 91125, USA
(Received 16 March 2005 / Accepted 10 April 2005)
Abstract
According to the unified scheme, AGN are surrounded by a dust-torus,
and the observed diversity of AGN properties results from the
different orientations relative to our line of sight. The strong
resonance of silicate dust at 10
m is therefore, as expected,
seen in absorption towards many type-2 AGN. In type-1 AGN, it should
be seen in emission because the hot inner surface of the dust torus
becomes visible. However, this has not been observed so far, thus
challenging the unification scheme or leading to exotic modifications
of the dust-torus model. Here we report the discovery of the
10
m silicate feature in emission in two luminous quasars with
the Infrared Spectrograph of the Spitzer Space Telescope.
Key words: galaxies: active -- galaxies: nuclei -- galaxies: quasars: general -- galaxies: quasars: individual: 3C 249.1 -- galaxies: quasars: individual: 3C 351
SIMBAD Objects
© ESO 2005
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