{ "id": "1806.11444", "version": "v1", "published": "2018-06-29T14:37:08.000Z", "updated": "2018-06-29T14:37:08.000Z", "title": "The two Ultraluminous X-ray sources in the galaxy NGC 925", "authors": [ "F. Pintore", "L. Zampieri", "S. Mereghetti", "A. Wolter", "G. Rodríguez", "G. L. Israel", "P. Esposito", "S. Paiano", "G. Trinchieri", "P. Ochner" ], "comment": "Accepted on MNRAS with very minor comments, 7 pages, 5 figures, 1 table", "categories": [ "astro-ph.HE", "astro-ph.GA" ], "abstract": "NGC 925 ULX-1 and ULX-2 are two ultraluminous X-ray sources in the galaxy NGC 925, at a distance of 8.5 Mpc. For the first time, we analyzed high quality, simultaneous XMM-Newton and NuSTAR data of both sources. Although at a first glance ULX-1 resembles an intermediate mass black hole candidate (IMBH) because of its high X-ray luminosity ($(2$$-$$4)\\times10^{40}$ erg s$^{-1}$) and its spectral/temporal features, a closer inspection shows that its properties are more similar to those of a typical super-Eddington accreting stellar black hole and we classify it as a `broadened disc' ultraluminous X-ray source. Based on the physical interpretation of this spectral state, we suggest that ULX-1 is seen at small inclination angles, possibly through the evacuated cone of a powerful wind originating in the accretion disc. The spectral classification of ULX-2 is less certain, but we disfavour an IMBH accreting at sub-Eddington rates as none of its spectral/temporal properties can be associated to either the soft or hard state of Galactic accreting black hole binaries.", "revisions": [ { "version": "v1", "updated": "2018-06-29T14:37:08.000Z" } ], "analyses": { "keywords": [ "ultraluminous x-ray source", "galaxy ngc", "accreting black hole binaries", "accreting stellar black hole", "super-eddington accreting stellar black" ], "note": { "typesetting": "TeX", "pages": 7, "language": "en", "license": "arXiv", "status": "editable" } } }