Journal
ASTROPHYSICAL JOURNAL
Volume 716, Issue 1, Pages 739-745Publisher
IOP PUBLISHING LTD
DOI: 10.1088/0004-637X/716/1/739
Keywords
cosmic background radiation; cosmology: observations; galaxies: clusters: individual (RXJ1347-1145)
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Funding
- STFC [ST/G002711/1] Funding Source: UKRI
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The most X-ray luminous cluster known, RXJ1347-1145 (z = 0.45), has been the object of extensive study across the electromagnetic spectrum. We have imaged the Sunyaev-Zel'dovich effect (SZE) at 90 GHz (lambda = 3.3 mm) in RXJ1347-1145 at 10 '' resolution with the 64 pixel MUSTANG bolometer array on the Green Bank Telescope, confirming a previously reported strong, localized enhancement of the SZE 20 '' to the southeast of the center of X-ray emission. This enhancement of the SZE has been interpreted as shock-heated (>20 keV) gas caused by an ongoing major (low mass ratio) merger event. Our data support this interpretation. We also detect a pronounced asymmetry in the projected cluster pressure profile, with the pressure just east of the cluster core similar to 1.6 x higher than just to the west. This is the highest resolution image of the SZE made to date.
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