X-ray Surface Brightness Fluctuations and ICM Physics

Details X-ray Surface Brightness Fluctuations and ICM Physics X-ray Surface Brightness Fluctuations and ICM Physics

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011scgg.conf....5c&link_type=abstract

"Structure in Clusters and Groups of Galaxies in the Chandra Era, 2011 Chandra Science Workshop held July 12-14, 2011. Edited by

Physics

Scientific paper

Chandra angular resolution provides exquisitely detailed X-ray images of nearby clusters and groups. Substructure seen in these images reflects the complexity of ICM physics, including thermal conduction, viscosity, magnetic fields, perturbations in gravitational potential and presence of gas motions. The results of the analysis of few brightest clusters are presented.

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