{ "id": "1411.7212", "version": "v1", "published": "2014-11-26T12:58:22.000Z", "updated": "2014-11-26T12:58:22.000Z", "title": "The slim-disk state of the ultraluminous X-ray source in M83", "authors": [ "Roberto Soria", "K. D. Kuntz", "Knox S. Long", "William P. Blair", "Paul P. Plucinsky", "P. Frank Winkler" ], "comment": "11 pages, accepted by the Astrophysical Journal", "categories": [ "astro-ph.HE" ], "abstract": "The transient ULX in M83 that went into outburst in or shortly before 2010 is still active. Our new XMM-Newton spectra show that it has a curved spectrum typical of the upper end of the high/soft state or slim-disk state. It appears to be spanning the gap between Galactic stellar-mass black holes and the ultraluminous state, at X-ray luminosities $\\approx (1$-$3) \\times 10^{39}$ erg s$^{-1}$ (a factor of two lower than in the 2010-2011 Chandra observations). From its broadened disk-like spectral shape at that luminosity, and from the fitted inner-disk radius and temperature, we argue that the accreting object is an ordinary stellar-mass black hole with $M \\sim$$10$-$20 M_{\\odot}$. We suggest that in the 2010-2011 Chandra observations, the source was seen at a higher accretion rate, resulting in a power-law-dominated spectrum with a soft excess at large radii.", "revisions": [ { "version": "v1", "updated": "2014-11-26T12:58:22.000Z" } ], "analyses": { "keywords": [ "ultraluminous x-ray source", "slim-disk state", "chandra observations", "galactic stellar-mass black holes", "ordinary stellar-mass black hole" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/0004-637X/799/2/140", "journal": "The Astrophysical Journal", "year": 2015, "month": "Feb", "volume": 799, "number": 2, "pages": 140 }, "note": { "typesetting": "TeX", "pages": 11, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1330260, "adsabs": "2015ApJ...799..140S" } } }