A parametric physical model for the intracluster medium and its use in joint SZ/X-ray analyses of galaxy clusters A parametric physical model for the ICM (2011)
Attributed to:
Radio Experimental Cosmology at Oxford
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1111/j.1365-2966.2010.17447.x
Publication URI: http://dx.doi.org/10.1111/j.1365-2966.2010.17447.x
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 1