A textbook example of ram-pressure stripping in the Hydra A/A780 cluster
S. De Grandi, D. Eckert, S. Molendi, M. Girardi, E. Roediger, M., Gaspari, F. Gastaldello, S. Ghizzardi, M. Nonino, M. Rossetti

TL;DR
This paper reports the discovery of an infalling galaxy group in Hydra A, showcasing ram-pressure stripping effects through deep X-ray observations, and compares the findings with numerical simulations to enhance understanding of the process.
Contribution
The study provides detailed observational evidence of ram-pressure stripping in a galaxy group, aligning with simulations and offering insights into cluster growth mechanisms.
Findings
Detection of a galaxy group 1.1 Mpc from Hydra A core
Identification of a 760 kpc gas wake trailing the group
Temperature of stripped gas is about half of surrounding plasma
Abstract
In the current epoch, one of the main mechanisms driving the growth of galaxy clusters is the continuous accretion of group-scale halos. In this process, the ram pressure applied by the hot intracluster medium on the gas content of the infalling group is responsible for stripping the gas from its dark-matter halo, which gradually leads to the virialization of the infalling gas in the potential well of the main cluster. Using deep wide-field observations of the poor cluster Hydra A/A780 with XMM-Newton and Suzaku, we report the discovery of an infalling galaxy group 1.1 Mpc south of the cluster core. The presence of a substructure is confirmed by a dynamical study of the galaxies in this region. A wake of stripped gas is trailing behind the group over a projected scale of 760 kpc. The temperature of the gas along the wake is constant at kT ~ 1.3 keV, which is about a factor of two less…
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