A detached double X-ray tail in the merging galaxy cluster Z8338 with a large double tail
Chong Ge, Ming Sun, Paul E. J. Nulsen, Craig Sarazin, Maxim, Markevitch, Gerrit Schellenberger

TL;DR
This paper reports the discovery of two large, double X-ray tails in galaxy cluster Z8338, revealing complex gas stripping and merger processes, with implications for cool core survival and magnetic field effects.
Contribution
First detailed observation of double X-ray tails in a galaxy cluster, highlighting cool core displacement, stability mechanisms, and merger dynamics.
Findings
Detached tail extended at least 250 kpc
Magnetic field of a few μG suppresses hydrodynamic instability
Cool core temperature increases from 0.9 keV to 1.6 keV
Abstract
When subhalos infall into galaxy clusters, their gas content is ram pressure stripped by the intracluster medium (ICM) and may turn into cometary tails. We report the discovery of two spectacular X-ray double tails in a single galaxy cluster, Z8338, revealed by 70 ks Chandra observations. The brighter one, with an X-ray bolometric luminosity of , is a detached tail stripped from the host halo and extended at least 250 kpc in projection. The head of the detached tail is a cool core with the front tip of the cold front 30 kpc away from the nucleus of its former host galaxy. The cooling time of the detached cool core is Gyr. For the detached gas, the gravity of the once-associated dark matter halo further enhances the Rayleigh-Taylor (RT) instability. From its survival, we find that a magnetic field of a few G is required to…
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