The XMM-Newton long look of NGC 1365: lack of a high/soft state in its ultraluminous X-ray sources

Details The XMM-Newton long look of NGC 1365: lack of a high/soft state in its ultraluminous X-ray sources The XMM-Newton long look of NGC 1365: lack of a high/soft state in its ultraluminous X-ray sources

2009-01-23

arxiv.org/abs/0901.3750v1

Astrophys.J.695:1614-1622,2009

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

9 pages, accepted by ApJ

Scientific paper

10.1088/0004-637X/695/2/1614

Based on our long (~ 300 ks) 2007 XMM-Newton observation of the Seyfert galaxy NGC 1365, we report here on the spectral and timing behaviour of two ultraluminous X-ray sources, which had previously reached isotropic X-ray luminosities L_X ~ 4 x 10^{40} erg/s (0.3-10 keV band). In 2007, they were in a lower state (L_X ~ 5 x 10^{39} erg/s, and L_X ~ 1.5 x 10^{39} erg/s for X1 and X2, respectively). Their X-ray spectra were dominated by power-laws with photon indices Gamma ~ 1.8 and Gamma ~ 1.2, respectively. Thus, their spectra were similar to those at their outburst peaks. Both sources have been seen to vary by a factor of 20 in luminosity over the years, but their spectra are always dominated by a hard power-law; unlike most stellar-mass BHs, they have never been found in a canonical high/soft state dominated by a standard disk. The lack of a canonical high/soft state seems to be a common feature of ULXs. We speculate that the different kind of donor star and/or a persistently super-Eddington accretion rate during their outbursts may prevent accretion flows in ULXs from settling into steady standard disks.

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