Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010head...11.0401s&link_type=abstract
American Astronomical Society, HEAD meeting #11, #4.01; Bulletin of the American Astronomical Society, Vol. 41, p.655
Astronomy and Astrophysics
Astronomy
Scientific paper
Some recent results on the interaction of the hot, X-ray emitting gas, cooler gaseous phases, dust, and radio plasma in the brightest cluster galaxies at the centers of cool core clusters of galaxies will be presented. The combination of low frequency radio images and sensitive X-ray observations shows that interactions between radio sources and the gas in clusters, groups, and individual galaxies are very common, and that the radio sources may have higher total energies than had been previously assumed. The results of a Chandra survey of the X-ray properties of a complete sample of bright X-ray clusters will be summarized. Finally, recent observations of cool gas and dust in the central galaxies of cool core clusters from the Science Demonstration Phase of a Herschel Key Project will be presented.
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