Another Interpretation of the Power-law type Spectrum of an Ultraluminous Compact X-ray Source in IC 342

Details Another Interpretation of the Power-law type Spectrum of an Ultraluminous Compact X-ray Source in IC 342 Another Interpretation of the Power-law type Spectrum of an Ultraluminous Compact X-ray Source in IC 342

2002-09-06

arxiv.org/abs/astro-ph/0209113v2

Mon.Not.Roy.Astron.Soc. 337 (2002) L11

Astronomy and Astrophysics

Astrophysics

5 pages, 3 figures and 1 table; accepted for publication for MNRAS letter

Scientific paper

10.1046/j.1365-8711.2002.06043.x

The ultraluminous compact X-ray sources (ULXs) generally show a curving spectrum in the 0.7--10 keV ASCA bandpass, which looks like a high temperature analogue of the disk dominated high/soft state spectra seen in Galactic black hole binaries (BHBs) at high mass accretion rates. Several ULXs have been seen to vary, and to make a transition at their lowest luminosity to a spectrum which looks more like a power law. These have been previously interpreted as the analogue of the power law dominated low/hard state in Galactic BHBs. However, the ULX luminosity at which the transition occurs must be at least 10--50 per cent of the Eddington limit assuming that their highest luminosity phase corresponds to the Eddington limit, while for the Galactic BHBs the high/soft--low/hard transition occurs at a few per cent of the Eddington limit. Here we show that the apparently power law spectrum in a ULX in IC342 can be equally well fit over the ASCA bandpass by a strongly Comptonised optically thick accretion disk with the maximum temperature of ~1 keV. Recent work on the Galactic BHBs has increasingly shown that such components are common at high mass accretion rates, and that this often characterises the very high (or anomalous) state. Thus we propose that the power law type ULX spectra are not to be identified with the low/hard state, but rather represent the Comptonisation dominated very high/anomalous state in the Galactic BHBs.

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