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A&A 442, L39-L43 (2005)
DOI: 10.1051/0004-6361:200500185
Letter
Spitzer IRS spectroscopy of 3CR radio galaxies and quasars: testing the unified schemes
M. Haas1, R. Siebenmorgen2, B. Schulz3, E. Krügel4 and R. Chini11 Astronomisches Institut, Ruhr-Universität, Universitätsstr. 150 / NA7, 44780 Bochum, Germany
e-mail: haas@astro.rub.de
2 European Southern Observatory, Karl-Schwarzschildstr. 2, 85748 Garching b. München, Germany
3 IPAC, California Institute of Technology (Caltech), Pasadena, CA 91125, USA
4 Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, Postfach 2024, 53010 Bonn, Germany
(Received 18 July 2005 / Accepted 11 September 2005)
Abstract
With the Spitzer Space Telescope Infrared Spectrograph (IRS)
we have observed seven powerful FR 2 radio galaxies and seven
quasars. Both samples, the galaxies and the quasars,
are comparable in isotropic 178 MHz luminosity
(10
W/Hz
W/Hz)
and in redshift range (0.05
z
1.5).
We find for both samples similar distributions in the luminosity ratios of high- to
low-excitation lines
([NeV]
/ [NeII]
) and of
high-excitation line to radio power
([NeV]
/
).
This solves the long debate about the apparent
difference of quasars and radio galaxies in favor of the
orientation-dependent unified schemes.
Furthermore, the luminosity ratio
[OIII]
/ [OIV]
of most galaxies is by a factor of ten
lower than that of the quasars. This suggests
that the optical emission from the
central NLR is essentially absorbed (
3)
in the powerful FR 2 galaxies and that the [OIII]
luminosity
does not serve as isotropic tracer for testing the unified schemes.
Key words: galaxies: active -- galaxies: nuclei -- galaxies: quasars: general -- infrared: galaxies
SIMBAD Objects
© ESO 2005
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