-
Articles citing this article
-
Same authors
- Recommend this article
- Download citation
- Alert me if this article is cited
- Alert me if this article is corrected
|
||||||||||||||||||
A&A 445, 115-122 (2006)
DOI: 10.1051/0004-6361:20054121
MAMBO 1.25 mm observations of 3CR quasars at z ~ 1.5: on the debate of the unified schemes
M. Haas1, R. Chini1, S. A. H. Müller1, F. Bertoldi2 and M. Albrecht31 Astronomisches Institut, Ruhr-Universität Bochum (AIRUB), Universitätsstr. 150 / NA7, 44780 Bochum, Germany
e-mail: haas@astro.rub.de
2 Radioastronomisches Institut, Universität Bonn, Auf dem Hügel 71, 53121 Bonn, Germany
3 Instituto de Astronomía, Universidad Católica del Norte, Avenida Angamos 0610, Antofagasta, Chile
(Received 16 December 2004 / Accepted 2 September 2005 )
Abstract
In order to explore the nature of the 850
m flux difference between
powerful radio galaxies and steep radio-spectrum quasars
at
reported by Willott et al. (2002), we have observed 9 sources from their sample of 11 quasars at 1.25 mm.
For 7 sources the 1.25 mm fluxes
are much brighter than one would expect from a purely thermal dust model
fitted to the submm data,
providing
evidence for the synchrotron nature of the observed 1.25 mm radiation.
If we extrapolate a power-law synchrotron spectrum to
shorter wavelengths, then for 6 of the 9 sources
also the 850
m fluxes are dominated by synchrotron
radiation.
We discuss how far the (sub)-millimetre data can be interpreted
in accordance with the
orientation-dependent unified schemes for powerful
radio galaxies and quasars.
In this case the results challenge the reported evidence for the
receding torus model and for
the evolutionary trend of a declining dust
luminosity with increasing projected size of the radio lobes.
Key words: galaxies: fundamental parameters -- galaxies: photometry -- galaxies: quasars: general -- infrared: galaxies
SIMBAD Objects
© ESO 2005
| What is OpenURL? |
- If your librarian has set up your subscription with an OpenURL resolver, OpenURL links appear automatically on the abstract pages.
- You can define your own OpenURL resolver with your EDPS Account. In this case your choice will be given priority over that of your library.
- You can use an add-on for your browser (Firefox or I.E.) to display OpenURL links on a page (see http://www.openly.com/openurlref/). You should disable this module if you wish to use the OpenURL server that you or your library have defined.

BibSonomy
CiteUlike
Connotea
Del.icio.us
Digg
Facebook