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Issue A&A
Volume 445, Number 1, January I 2006
Page(s) 115 - 122
Section Extragalactic astronomy
DOI http://dx.doi.org/10.1051/0004-6361:20054121



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. Albrecht3

1  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 $\mu$m flux difference between powerful radio galaxies and steep radio-spectrum quasars at $z\sim 1.5$ 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 $\mu$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

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© ESO 2005


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