2022/09/21 by E. Molina, Molina, E., López-Oramas, A. +4
Physics and Astronomy · #Arithmetic #Astronomy #Astrophysical Phenomena and Observations #Astrophysics #Astrophysics and Cosmic Phenomena #Binary number #Degenerate energy levels #Gamma ray #Gamma-ray astronomy #Gamma-ray bursts and supernovae #MAGIC (telescope) #Nuclear physics #Physics #Radiation
paper · pdf · doi:10.48550/arxiv.2209.10226
published in arXiv (Cornell University) (Cornell University)
openalex publication_date 2022/09/21 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
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.