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               <dc:title>NIR spectral classification of the companion in the gamma-ray binary HESS J1832-093 as an O6 V star</dc:title>
               <dc:creator>Van Soelen, Brian</dc:creator>
               <dc:creator>Bordas Coma, Pol</dc:creator>
               <dc:creator>Negueruela, Ignacio</dc:creator>
               <dc:creator>De Oña Wilhelmi, E.</dc:creator>
               <dc:creator>Papitto, A.</dc:creator>
               <dc:creator>Ribó Gomis, Marc</dc:creator>
               <dc:subject>Estels de neutrons</dc:subject>
               <dc:subject>Estels binaris</dc:subject>
               <dc:subject>Raigs X</dc:subject>
               <dc:subject>Neutron stars</dc:subject>
               <dc:subject>Double stars</dc:subject>
               <dc:subject>X-rays</dc:subject>
               <dc:description>HESS 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.</dc:description>
               <dc:date>2025-04-08T16:48:18Z</dc:date>
               <dc:date>2025-04-08T16:48:18Z</dc:date>
               <dc:date>2024-03-01</dc:date>
               <dc:date>2025-04-08T16:48:18Z</dc:date>
               <dc:type>info:eu-repo/semantics/article</dc:type>
               <dc:type>info:eu-repo/semantics/publishedVersion</dc:type>
               <dc:relation>Reproducció del document publicat a: https://doi.org/10.1093/mnrasl/slae007</dc:relation>
               <dc:relation>Monthly Notices of the Royal Astronomical Society: Letters, 2024, vol. 529, num.1</dc:relation>
               <dc:relation>https://doi.org/10.1093/mnrasl/slae007</dc:relation>
               <dc:rights>(c)  Van Soelen, B. et al., 2024</dc:rights>
               <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
               <dc:publisher>Royal Astronomical Society</dc:publisher>
               <dc:source>Articles publicats en revistes (Física Quàntica i Astrofísica)</dc:source>
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