Van Soelen, BrianBordas Coma, PolNegueruela, IgnacioDe Oña Wilhelmi, E.Papitto, A.Ribó Gomis, Marc2025-04-082025-04-082024-03-011745-3933https://hdl.handle.net/2445/220343HESS J1832-093 is a member of the rare class of gamma-ray binaries, as recently confirmed by the detection of orbitally modulated X-ray and gamma-ray emission with a period of ~86 d. The spectral type of the massive companion star has been difficult to retrieve as there is no optical counterpart, but the system is coincident with a near-infrared source. Previous results have shown that the infrared counterpart is consistent with an O or B-type star, but a clear classification is still lacking. We observed the counterpart twice, in 2019 and 2021, with the X-Shooter spectrograph operating on the Very Large Telescope (VLT). The obtained spectra classify the counterpart as an O6 V-type star. We estimate a distance to the source of 6.7 ± 0.5 kpc, although this estimate can be severely affected by the high extinction towards the source. This new O6 V classification for the companion star in HESS J1832-093 provides further support to an apparent grouping around a given spectral type for all discovered gamma-ray binaries that contain an O-type star. This may be due to the interplay between the initial mass function and the wind momentum-luminosity relation.1 p.application/pdfeng(c) Van Soelen, B. et al., 2024Estels de neutronsEstels binarisRaigs XNeutron starsDouble starsX-raysinfo:eu-repo/semantics/article7447462025-04-08info:eu-repo/semantics/openAccess