Soria, R; Zampieri, L; Zane, S; Wu, K; (2011) X-ray study of HLX1: intermediate-mass black hole or foreground neutron star? Monthly Notices of the Royal Astronomical Society , 410 (3) 1886 - 1894. 10.1111/j.1365-2966.2010.17572.x.

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Abstract

We re-assess the XMM-Newton and Swift observations of HLX1, to examine the evidence for its identification as an intermediate-mass black hole. We show that the X-ray spectral and timing properties are equally consistent with an intermediate-mass black hole in a high state, or with a foreground neutron star with a luminosity of about a few times 1E32 erg/s ~ 1E-6 LEdd, located at a distance of about 1.5 to 3 kpc. Contrary to previously published results, we find that the X-ray spectral change between the two XMM-Newton observations of 2004 and 2008 (going from power-law dominated to thermal dominated) is not associated with a change in the X-ray luminosity. The thermal component becomes more dominant (and hotter) during the 2009 outburst seen by Swift, but in a way that is consistent with either scenario.

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