no code implementations • 28 Dec 2020 • K. Rajpurohit, G. Brunetti, A. Bonafede, R. J. van Weeren, A. Botteon, F. Vazza, M. Hoeft, C. J. Riseley, E. Bonnassieux, M. Brienza, W. R. Forman, H. J. A. Röttgering, A. S. Rajpurohit, N. Locatelli, T. W. Shimwell, R. Cassano, G. Di Gennaro, M. Brüggen, D. Wittor, A. Drabent, A. Ignesti
The compelling evidence for a steep spectral index, the existence of a spectral break above 1. 5 GHz, and the dependence of radio and X-ray surface brightness correlation on frequency are interpreted in the context of turbulent reacceleration models.
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
no code implementations • 6 Jul 2020 • A. Jimenez-Gallardo, F. Massaro, M. A. Prieto, V. Missaglia, C. Stuardi, A. Paggi, F. Ricci, R. P. Kraft, E. Liuzzo, G. R. Tremblay, S. A. Baum, C. P. O'Dea, B. J. Wilkes, J. Kuraszkiewicz, W. R. Forman, D. E. Harris
We present the analysis of nine radio sources belonging to the Third Cambridge Revised catalog (3CR) observed with $Chandra$ during Cycle 20 in the redshift range between 1. 5 and 2. 5.
Astrophysics of Galaxies High Energy Astrophysical Phenomena
