IGR J17329-2731

IGR J17329-2731 is an astronomical object classified as a high-mass X-ray binary star system located in the constellation of Scorpius. It was identified by the International Gamma-Ray Observatory (IGR) and has been the subject of various studies due to its X-ray emissions. Typically, high-mass X-ray binaries consist of a massive star and a compact object, such as a neutron star or black hole, that is accreting matter from the massive companion.