An international team of astronomers has performed multiwavelength observations of a gamma-ray binary system known as HESS J0632+057. Results of the observational campaign, presented July 31 on the pre-print server arXiv, shed more light on the nature of this binary.
Gamma-ray binaries consist of a massive OB-type star in orbit with a compact object like a neutron star or black hole. Some of them emit a significant amount of radiation in very high-energy (TeV) and are therefore known as TeV gamma-ray binaries (TGBs).
TGBs exhibit diverse high-energy phenomena driven by interactions between the two components. Given that these sources are extremely rare, astronomers are especially interested in exploring them in detail, which could help us better understand their mysterious nature.