A Polytropic b-Model to Fit the X-ray Surface Brightness of Clusters of Galaxies

Details A Polytropic b-Model to Fit the X-ray Surface Brightness of Clusters of Galaxies A Polytropic b-Model to Fit the X-ray Surface Brightness of Clusters of Galaxies

Mar 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000lssx.proc..353e&link_type=toc

Large Scale Structure in the X-ray Universe, Proceedings of the 20-22 September 1999 Workshop, Santorini, Greece, eds. Plionis,

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