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The central radio source in the NGC 383 group: jet - IGM interaction ?

Stefanie Komossa·Hans Boehringer
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Abstract

The NGC 383 group is a rich group of galaxies that harbours the central radio source 3C 31 = NGC 383. After presenting results from the X-ray analysis of the extended intra-group medium and the central radio galaxy, we discuss the spatial morphology of X-ray emitting gas as compared to the radio plasma and perform a comparison of the pressures of both components.

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Stefanie Komossa, Hans Boehringer. 1999-05-05. The central radio source in the NGC 383 group: jet - IGM interaction ?. https://arxiv.org/abs/astro-ph/9905034

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