{ "id": "2108.08039", "version": "v1", "published": "2021-08-18T08:42:06.000Z", "updated": "2021-08-18T08:42:06.000Z", "title": "Investigating the true nature of three hard X-ray sources", "authors": [ "Manuela Molina", "Angela Malizia", "Nicola Masetti", "Loredana Bassani", "Angela Bazzano", "Anthony J. Bird", "Mariateresa Fiocchi", "Eliana Palazzi", "Pietro Ubertini" ], "comment": "11 pages, 8 figures, accepted for publication on MNRAS", "categories": [ "astro-ph.HE" ], "abstract": "Many of the new high energy sources discovered both by INTEGRAL/IBIS and Swift/BAT have been characterised thanks to extensive, multi-band follow-up campaigns, but there are still objects whose nature remains to be asserted. In this paper we investigate the true nature of three high energy sources, IGR J12134-6015, IGR J16058-7253 and Swift J2037.2+4151, employing multiwavelength data from the NIR to the X-rays. Through Gaia and ESO-VLT measurements and through Swift/XRT X-ray spectral analysis, we re-evaluate the classification for IGR J12134-6015, arguing that the source is a Galactic object and in particular a Cataclysmic Variable. We were able to confirm, thanks to NuSTAR observations, that the hard X-ray emission detected by INTEGRAL/IBIS and Swift/BAT from IGR J16058-7253 is coming from two Seyfert 2 galaxies which are both counterparts for this source. Through optical and X-ray spectral analysis of Swift J2037.2+4151 we find that this source is likely part of the rare and peculiar class of Symbiotic X-ray binaries and displays flux and spectral variability as well as interesting spectral features, such as a blending of several emission lines around the iron line complex.", "revisions": [ { "version": "v1", "updated": "2021-08-18T08:42:06.000Z" } ], "analyses": { "keywords": [ "hard x-ray sources", "true nature", "high energy sources", "swift/xrt x-ray spectral analysis", "symbiotic x-ray binaries" ], "note": { "typesetting": "TeX", "pages": 11, "language": "en", "license": "arXiv", "status": "editable" } } }