Abstract
The radio and x-ray emission in nearby early type galaxies are compared. The results indicate that there is a correlation between the x-ray and the radio luminosities, although with a very large scatter. Part of this scatter might be reduced with better radio data (for the x-ray data, we will have to wait a while), but most of it is probably intrinsic to the data, and indicates a rather complex relation between these two quantities. Sources with low radio luminosity could be effectively confined within the optical galaxy by the hot gas radiating in x-rays. For galaxies with Lr > 1029 ergs s-1Hz-1 confinement is no longer viable.
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© 1988 Kluwer Academic Publishers
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Trinchieri, G. (1988). Radio and X-Ray Emission in Early Type Galaxies. In: Fabian, A.C. (eds) Cooling Flows in Clusters and Galaxies. NATO ASI Series, vol 229. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-2953-1_33
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DOI: https://doi.org/10.1007/978-94-009-2953-1_33
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-7828-3
Online ISBN: 978-94-009-2953-1
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