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arXiv · 1308.1282

X-ray variability and energy spectra from NGC5408 X-1 with XMM-Newton

M. D. Caballero-Garcia·T. Belloni·A. Wolter
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Abstract

The notion of source states characterizing the X-ray emission from black hole binaries has revealed to be a very useful tool to disentangle the complex spectral and aperiodic phenomenology displayed by those classes of accreting objects. We seek to use the same tools for Ultra-Luminous X-ray (ULX) sources. We analyzed the data from the longest observations obtained from the ULX source in NGC 5408 (NGC 5408 X-1) taken by XMM-Newton. We performed a study of the timing and spectral properties of the source. In accordance with previous studies on similar sources, the intrinsic energy spectra of the source are well described by a cold accretion disc emission plus a curved high-energy emission component. We studied the broad-band noise variability of the source and found an anti-correlation between the root mean square variability in the 0.0001-0.2Hz and intensity, similarly to what is observed in black-hole binaries during the hard states. We discuss the physical processes responsible for the X-ray features observed and suggest that NGC 5408 X-1 harbors a black hole accreting in an unusual bright hard-intermediate state.

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M. D. Caballero-Garcia, T. Belloni, A. Wolter. 2013-08-06. X-ray variability and energy spectra from NGC5408 X-1 with XMM-Newton. https://doi.org/10.1093/mnras%2Fstt1479

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