A combined LOFAR and XMM-Newton analysis of the disturbed cluster PSZ2G113.91-37.01
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Published:2023-11-22
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ISSN:0004-6361
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Container-title:Astronomy & Astrophysics
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language:
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Short-container-title:A&A
Author:
Campitiello M.G.,Bonafede A.,Botteon A.,Lovisari L.,Ettori S.,Brunetti G.,Gastaldello F.,Rossetti M.,Cassano R.,Ignesti A.,van Weeren R.J.,Brüggen M.,Hoeft M.
Abstract
In this work, we investigated the interplay between the X-ray and radio emission of the cluster PSZ2G113.91-37.01 ($z = 0.371$) using the high-quality XMM-Newton observations of the Cluster HEritage project with XMM-Newton - Mass Assembly and Thermodynamics at the Endpoint of structure formation (CHEX-MATE), and the images of the LOFAR Two-meter Sky Survey-Data release 2 (LoTSS-DR2). The cluster is undergoing a merger along the north-south axis, and shows a central radio halo and two radio relics, one in the southern and one in the northern regions. The analysis of the intracluster medium (ICM) distribution revealed the presence of a northern surface brightness (SB) jump associated to the merger event. By extracting spectra across this discontinuity, we classified the edge as a cold front. Furthermore, we made use of upgraded Giant Metrewave Radio Telescope observations that allowed us to perform a spectral analysis of the G113 radio emission. We found evidence of re-acceleration of particles in the northern relic, and we measured an associated Mach number of $ M as inferred from radio observations. We then performed a point-to-point analysis of the X-ray and radio emission both in the halo and in the northern relic regions. We found a strong correlation for the halo and an anti-correlation for the relic. The former behaviour is in agreement with previous studies. The relic anti-correlation is likely related to the reverse radial distribution of the X-ray (increasing towards the cluster centre) and radio (decreasing towards the cluster centre) emissions. Finally, we performed a point-to-point analysis of the radio emission and the residuals obtained by subtracting a double beta model to the X-ray emission. We found a strong correlation between the two quantities. This behaviour suggests the presence of a connection between the process responsible for the radio emission and the one that leaves fluctuations in the X-ray observations.
Subject
Space and Planetary Science,Astronomy and Astrophysics
Cited by
1 articles.
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