no code implementations • 12 Feb 2021 • G. Di Gennaro, R. J. van Weeren, L. Rudnick, M. Hoeft, M. Brüggen, D. Ryu, H. J. A. Röttgering, W. Forman, A. Stroe, T. W. Shimwell, R. P. Kraft, C. Jones, D. N. Hoang
For the first time in a radio relic, we observe a decreasing polarization fraction in the downstream region.
Astrophysics of Galaxies Cosmology and Nongalactic Astrophysics
no code implementations • 10 Jul 2020 • Y. Su, Y. Zhang, G. Liang, J. A. ZuHone, D. J. Barnes, N. B. Jacobs, M. Ntampaka, W. R. Forman, P. E. J. Nulsen, R. P. Kraft, C. Jones
From this analysis, we observe that the network has utilized regions from cluster centers out to r~300 kpc and r~500 kpc to identify CC and NCC clusters, respectively.
Cosmology and Nongalactic Astrophysics
1 code implementation • 2 May 2017 • W. Forman, E. Churazov, C. Jones, S. Heinz, R. Kraft, A. Vikhlinin
A deep Chandra observation of M87 exhibits an approximately circular shock front (13 kpc radius, in projection) driven by the expansion of the central cavity (filled by the SMBH with relativistic radio-emitting plasma) with projected radius $\sim$1. 9 kpc.
Astrophysics of Galaxies High Energy Astrophysical Phenomena
