http://arxiv.org/abs/2209.10226
X-ray and gamma-ray binaries are systems consisting of a compact object and normally a non-degenerate companion star. Most of these sources have been shown to emit radiation in a broad frequency range, from radio up to X-rays and sometimes gamma rays. We report on recent results in very high-energy gamma rays above 100 GeV obtained by the MAGIC Collaboration for the Galactic X-ray binaries MAXI J1820+070 and 1A 0535+262, and the gamma-ray binary HESS J0632+057. Multiwavelength data at lower energies are also provided for a better contextualisation of the sources.
E. Molina, A. López-Oramas, D. Hadasch, et. al.
Thu, 22 Sep 22
3/65
Comments: 9 pages, 3 figures. Proceedings of the ICRC 2021