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A Rare, Strong Shock Front in the Merging Cluster SPT-CLJ 2031-4037

Authors :
Purva Diwanji
Stephen A. Walker
M. S. Mirakhor
Source :
The Astrophysical Journal, Vol 969, Iss 2, p 115 (2024)
Publication Year :
2024
Publisher :
IOP Publishing, 2024.

Abstract

We present our findings from the new deep Chandra observations (256 ks) of the merging galaxy cluster SPT-CLJ 2031-4037 at z = 0.34. Our observations reveal intricate structures seen in a major merger akin to the Bullet Cluster. The X-ray data confirm the existence of two shock fronts, one to the northwest and one to the southeast, by directly measuring the temperature jump of gas across the surface brightness edges. The stronger shock front in the northwest has a density jump of 3.16 ± 0.34 across the sharp surface brightness edge and Mach number $M={3.36}_{-0.48}^{+0.87}$ , which makes this cluster one of the rare merging systems with a Mach number M > 2. We use the northwestern shock to compare two models for shock heating—the instant heating model and the Coulomb collisional heating model—and we determine that the temperatures across the shock front agree with the Coulomb collisional model of heating. For the shock front in the southeastern region, we find a density jump of 1.53 ± 0.14 and a Mach number of $M={1.36}_{-0.08}^{+0.09}$ .

Details

Language :
English
ISSN :
15384357
Volume :
969
Issue :
2
Database :
Directory of Open Access Journals
Journal :
The Astrophysical Journal
Publication Type :
Academic Journal
Accession number :
edsdoj.25e9405792f4be89f3a9df425de1330
Document Type :
article
Full Text :
https://doi.org/10.3847/1538-4357/ad47f8