Abstract
We present deep Chandra observations of A3411–12, a remarkable merging cluster that hosts the most compelling evidence for electron reacceleration at cluster shocks to date. Using the scaling relation, we find r 500 ∼ 1.3 Mpc, , , and a gas mass of . The gas mass fraction within r 500 is . We compute the shock strength using density jumps to conclude that the Mach number of the merging subcluster is small ( ). We also present density, temperature, pseudo-pressure, and pseudo-entropy maps. Based on the pseudo-entropy map, we conclude that the cluster is undergoing a mild merger, consistent with the small Mach number. On the other hand, radio relics extend over Mpc scale in the A3411–12 system, which strongly suggests that a population of energetic electrons already existed over extended regions of the cluster.
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CITATION STYLE
Andrade-Santos, F., van Weeren, R. J., Di Gennaro, G., Wittman, D., Ryu, D., Lal, D. V., … Dawson, W. (2019). Chandra Observations of the Spectacular A3411–12 Merger Event. The Astrophysical Journal, 887(1), 31. https://doi.org/10.3847/1538-4357/ab4ce5
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