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MM Emission from Quasars

Published online by Cambridge University Press:  03 August 2017

R. Chini
R. Chini*
Affiliation:
Max-Planck-Institut für Radioastronomie Auf dem Hügel 69 D-5300 Bonn FRG

Abstract

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1.3mm continuum observations for a complete sample of optically selected southern quasars show that most objects have flux densities below ≈40mJy at that wavelength. This clearly indicates that previously claimed detections at Jy level are erroneous. The sample is divided into radio-quiet and radio-loud objects. While for the first group a thermal origin of the FIR emission is very likely the latter group shows energy distributions dominated by Synchrotron radiation.

Type
XIII- IRAS Ultraluminous Objects and Quasars
Information
Symposium - International Astronomical Union , Volume 146: Dynamics of Galaxies and their Molecular Cloud Distributions , 1991 , pp. 434 - 436
Copyright
Copyright © Kluwer 1991 

References

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