Radio Jets as a Probe of the Cooling Flow Environment View Full Text


Ontology type: schema:Chapter     


Chapter Info

DATE

1988

AUTHORS

D. M. Sumi , M. L. Norman , L. L. Smarr

ABSTRACT

We discuss the use of radio jets as a probe of the structure of cooling flows on length scales inaccessible to the currently available X-ray data. The radio structure of one such cooling flow galaxy, IC 1101, suggests a shock disruption of a supersonic beam. This type of radio structure is also found associated with other cooling flow galaxies. The shock disruption is discussed in terms of an interaction of the beam with the cooling flow environment. The current sophistication of these disruption mechanisms and of the radio observations does not compel one to favor one mechanism over another. Each mechanism, however, may be useful in studying the central regions of cooling flows. More... »

PAGES

257-261

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/978-94-009-2953-1_31

DOI

http://dx.doi.org/10.1007/978-94-009-2953-1_31

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1004562071


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