Synchrotron emission from a nearby zone of SgrA$^*$
High Energy Astrophysical Phenomena
2021-04-01 v3 Astrophysics of Galaxies
Abstract
Quasi-linear diffusion (QLD), driven by the cyclotron instability, is proposed as a mechanism for the possible generation of synchrotron emission in the nearby zone of SgrA. For physically reasonable parameters, the QLD, by causing non-zero pitch angle scattering lets electrons with the relativistic factors of the order of emit synchrotron radiation in the hard -ray spectral band keV.
Keywords
Cite
@article{arxiv.2103.01900,
title = {Synchrotron emission from a nearby zone of SgrA$^*$},
author = {G. Gogaberishvili and Z. N. Osmanov and S. M. Mahajan},
journal= {arXiv preprint arXiv:2103.01900},
year = {2021}
}
Comments
4 pages, 3 figures