Recent MAGIC results on Galactic binaries
Abstract
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.
- Publication:
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37th International Cosmic Ray Conference
- Pub Date:
- March 2022
- DOI:
- 10.22323/1.395.0786
- arXiv:
- arXiv:2209.10226
- Bibcode:
- 2022icrc.confE.786M
- Keywords:
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- Astrophysics - High Energy Astrophysical Phenomena
- E-Print:
- 9 pages, 3 figures. Proceedings of the ICRC 2021