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2011MNRAS.416..302P - Mon. Not. R. Astron. Soc., 416, 302-310 (2011/September-1)
A high-frequency study of the Sunyaev–Zel'dovich effect morphology in galaxy clusters.
PROKHOROV D.A., COLAFRANCESCO S., AKAHORI T., MILLION E.T., NAGATAKI S. and YOSHIKAWA K.
Abstract (from CDS):
We calculate relativistically corrected SZ intensity maps of a simulated, massive, merging galaxy cluster and of the massive, merging clusters 1E0657-558 (the Bullet cluster) and Abell 2219. The morphologies of the SZ intensity maps are remarkably different between 345 and 857 GHz for each merging cluster. We show that high-resolution imaging observations of the SZ intensity maps at these frequencies, obtainable with the LABOCA and HERSCHEL-SPIRE instruments, allow to fully exploit the astrophysical relevance of the predicted SZ morphological effect.
Abstract Copyright: 2011 The Authors Monthly Notices of the Royal Astronomical Society2011 RAS
Journal keyword(s): galaxies: cluster: general - cosmic background radiation
Simbad objects: 4
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