Structure formation in the current Universe operates through the accretion of group-scale systems onto massive clusters. The detection and study of such accreting systems is crucial to understand the build-up of the most massive virialized structures we see today. We report the discovery with XMM-Newton of an irregular X-ray substructure in the outskirts of the massive galaxy cluster Abell 2142. The tip of the X-ray emission coincides with a concentration of galaxies. The bulk of the X-ray emission of this substructure appears to be lagging behind the galaxies and extends over a projected scale of at least 800 kpc. The temperature of the gas in this region is 1.4 keV, which is a factor of ~4 lower than the surrounding medium and is typical of the virialized plasma of a galaxy group with a mass of a few 10^13 M☉. For this reason, we interpret this structure as a galaxy group in the process of being accreted onto the main dark-matter halo. The X-ray structure trailing behind the group is due to gas stripped from its original dark-matter halo as it moves through the intracluster medium (ICM). This is the longest X-ray trail reported to date. For an infall velocity of ~1200 km s-1 we estimate that the stripped gas has been surviving in the presence of the hot ICM for at least 600 Myr, which exceeds the Spitzer conduction timescale in the medium by a factor of ≳400. Such a strong suppression of conductivity is likely related to a tangled magnetic field with small coherence length and to plasma microinstabilities. The long survival time of the low-entropy intragroup medium suggests that the infalling material can eventually settle within the core of the main cluster.

The stripping of a galaxy group diving into the massive cluster A2142 / Eckert, D; Molendi, S; Owers, M; Gaspari, M; Venturi, T; Rudnick, L; Ettori, S; Paltani, S; Gastaldello, F; Rossetti, M. - In: ASTRONOMY & ASTROPHYSICS. - ISSN 1432-0746. - 570:(2014). [10.1051/0004-6361/201424259]

The stripping of a galaxy group diving into the massive cluster A2142

Gaspari M;
2014

Abstract

Structure formation in the current Universe operates through the accretion of group-scale systems onto massive clusters. The detection and study of such accreting systems is crucial to understand the build-up of the most massive virialized structures we see today. We report the discovery with XMM-Newton of an irregular X-ray substructure in the outskirts of the massive galaxy cluster Abell 2142. The tip of the X-ray emission coincides with a concentration of galaxies. The bulk of the X-ray emission of this substructure appears to be lagging behind the galaxies and extends over a projected scale of at least 800 kpc. The temperature of the gas in this region is 1.4 keV, which is a factor of ~4 lower than the surrounding medium and is typical of the virialized plasma of a galaxy group with a mass of a few 10^13 M☉. For this reason, we interpret this structure as a galaxy group in the process of being accreted onto the main dark-matter halo. The X-ray structure trailing behind the group is due to gas stripped from its original dark-matter halo as it moves through the intracluster medium (ICM). This is the longest X-ray trail reported to date. For an infall velocity of ~1200 km s-1 we estimate that the stripped gas has been surviving in the presence of the hot ICM for at least 600 Myr, which exceeds the Spitzer conduction timescale in the medium by a factor of ≳400. Such a strong suppression of conductivity is likely related to a tangled magnetic field with small coherence length and to plasma microinstabilities. The long survival time of the low-entropy intragroup medium suggests that the infalling material can eventually settle within the core of the main cluster.
2014
570
The stripping of a galaxy group diving into the massive cluster A2142 / Eckert, D; Molendi, S; Owers, M; Gaspari, M; Venturi, T; Rudnick, L; Ettori, S; Paltani, S; Gastaldello, F; Rossetti, M. - In: ASTRONOMY & ASTROPHYSICS. - ISSN 1432-0746. - 570:(2014). [10.1051/0004-6361/201424259]
Eckert, D; Molendi, S; Owers, M; Gaspari, M; Venturi, T; Rudnick, L; Ettori, S; Paltani, S; Gastaldello, F; Rossetti, M
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11380/1338436
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