Turbulence and Magnetic Fields in Clusters of Galaxies

Details Turbulence and Magnetic Fields in Clusters of Galaxies Turbulence and Magnetic Fields in Clusters of Galaxies

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ap%26ss.263...87s&link_type=abstract

Astrophysics and Space Science, v. 263, Issue 1/4, p. 87-90 (1998).

Astronomy and Astrophysics

Astrophysics

7

Scientific paper

We consider turbulence generated by galaxies moving transonically through the intracluster gas. We show that neither the gravitational drag nor the gas stripping from the galaxies are able, by themselves, to generate turbulence at a level required to feed the dynamo in the intracluster gas. Some implications for cluster radio halos are discussed.

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