Abstract
A qualitative description is given of spectral properties, dynamical behaviour and morphology of a selection of mainly southern radio galaxies which have been observed to have extended ionized gas in their vicinity. The question of the significance of this gas in relation to cooling flows is still very much an open one.
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© 1988 Kluwer Academic Publishers
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Danziger, I.J., Focardi, P. (1988). Characteristics of Extended Gas Around Radio 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_15
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DOI: https://doi.org/10.1007/978-94-009-2953-1_15
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