The slim-disk state of the ultraluminous X-ray source in M83
arXiv:1411.7212 · doi:10.1088/0004-637X/799/2/140
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 - erg s (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 -. 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.
11 pages, accepted by the Astrophysical Journal
References in corpus (9)
- Super-critically accreting stellar-mass black holes as ultraluminous X-ray sources
- XMM-Newton observations of the brightest Ultraluminous X-ray sources
- A mass of less than 15 solar masses for the black hole in an ultraluminous X-ray source
- Cepheid Distances to SNe Ia Host Galaxies based on a Revised Photometric Zero-Point of the HST-WFPC2 and New P-L Relations and Metallicity Corrections
- X-ray observations of ultraluminous X-ray sources
- Reprocessing of X-rays in the outer accretion disc of the black hole binary XTE J1817--330
- A Deep Chandra ACIS Survey of M83
- Bridging the gap between stellar-mass black holes and ultraluminous X-ray sources
- Irradiated, colour-temperature-corrected accretion discs in ultraluminous X-ray sources
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