Radio haloes, cluster mergers, and cooling flows

Details Radio haloes, cluster mergers, and cooling flows Radio haloes, cluster mergers, and cooling flows

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993mnras.263...31t&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 263, no. 1, p. 31-36.

Astronomy and Astrophysics

Astrophysics

120

Cooling Flows (Astrophysics), Galactic Clusters, Halos, Radio Emission, Relativistic Particles, Astronomical Models, Galactic Evolution, Interstellar Magnetic Fields, Radio Astronomy

Scientific paper

Radio haloes are rarely found in galaxy clusters with cooling flows, and those that are found are different from the canonical haloes such as that in the Coma cluster. I propose that the big cluster radio haloes are transient, being formed in large cluster mergers and then fading. The small haloes in cooling flows are a result of magnetic field compression and reacceleration of old relativistic electrons by the cooling flow.

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