Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/6830
Title: MACS J0553.4-3342: a young merging galaxy cluster caught through the eyes of Chandra and HST.
Authors: Pandge, M.B.
Bagchi, Joydeep
Sonkamble, S.S.
Parekh, Viral
+ 5 Co-authors
Keywords: galaxies clusters
Issue Date: Dec-2017
Publisher: Oxford University Press for The Royal Astronomical Society
Citation: Monthly Notices of the Royal Astronomical Society, 2017, Vol. 472, p2042-2053
Abstract: We present a detailed analysis of a young merging galaxy cluster MACS J0553.4−3342 (z=0.43) from Chandra X-ray and Hubble Space Telescope archival data. X-ray observations confirm that the X-ray emitting intra-cluster medium (ICM) in this system is among the hottest (average T = 12.1 ± 0.6 keV) and most luminous known. Comparison of X-ray and optical images confirms that this system hosts two merging subclusters SC1 and SC2, separated by a projected distance of about 650 kpc. The subcluster SC2 is newly identified in this work, while another subcluster (SC0), previously thought to be a part of this merging system, is shown to be possibly a foreground object. Apart from two subclusters, we find a tail-like structure in the X-ray image, extending to a projected distance of ∼1 Mpc, along the north-east direction of the eastern subcluster (SC1). From a surface brightness analysis, we detect two sharp surface brightness edges at ∼40 (∼320 kpc) and ∼80 arcsec (∼640 kpc) to the east of SC1. The inner edge appears to be associated with a merger-driven cold front, while the outer one is likely to be due to a shock front, the presence of which, ahead of the cold front, makes this dynamically disturbed cluster interesting. Nearly all the early-type galaxies belonging to the two subclusters, including their brightest cluster galaxies, are part of a well-defined red sequence.
Description: Open Access
URI: http://hdl.handle.net/2289/6830
ISSN: 0035-8711
1365-2966 - (online)
Alternative Location: http://adsabs.harvard.edu/abs/2017MNRAS.472.2042P
https://arxiv.org/abs/1701.00197
http://dx.doi.org/10.1093/mnras/stx2028
Copyright: 2017 The authors & the Royal Astronomical Society
Appears in Collections:Research Papers (A&A)

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