Lara-López, Maritza A.Zinchenko, Igor A.Pilyugin, Leonid S.Gunawardhana, Madusha L. P.López-Cruz, OmarO'Sullivan, Shane P.Feltre, AnnaRosado, MargaritaSánchez-Cruces, MónicaChevallard, JacopoDe Rossi, Maria EmiliaDib, SamiFritz, JacopoFuentes-Carrera, IsauraGarduño, Luis E.Ibar, Eduardo2022-11-302022-11-302021Maritza A. Lara-López et al 2021 ApJ 906 42http://repositoriobibliotecas.uv.cl/handle/uvscl/7384We present an analysis of the optical properties of three Ultra Luminous X-ray (ULX) sources identified in NGC 925. We use Integral field unit data from the George Mitchel spectrograph in the context of the Metal-THINGS survey. The optical properties for ULX-1 and ULX-3 are presented, while the spaxel associated with ULX-2 had a low S/N, which prevented its analysis. We also report the kinematics and dimensions of the optical nebula associated with each ULX using ancillary data from the PUMA Fabry–Perot spectrograph. A BPT analysis demonstrates that most spaxels in NGC 925 are dominated by star-forming regions, including those associated with ULX-1 and ULX-3. Using the resolved gas-phase metallicities, a negative metallicity gradient is found, consistent with previous results for spiral galaxies, while the ionization parameter tends to increase radially throughout the galaxy. Interestingly, ULX-1 shows a very low gas metallicity for its galactocentric distance, identified by two independent methods, while exhibiting a typical ionization. We find that such low gas metallicity is best explained in the context of the high-mass X-ray binary population, where the low-metallicity environment favors active Roche lobe overflows that can drive much higher accretion rates. An alternative scenario invoking accretion of a low-mass galaxy is not supported by the data in this region. Finally, ULX-3 shows both a high metallicity and ionization parameter, which is consistent with the progenitor being a highly accreting neutron star within an evolved stellar population region.© 2021. The American Astronomical Society. All rights reservedEMISSION LINE GALAXIESIONIZATIONCHEMICAL ABUNDANCESABUNDANCE RATIOSSPECTROSCOPYX-RAY SOURCESArticulo10.3847/1538-4357/abc892