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The aperiodic variability of the Ultraluminous X-ray source in NGC 5408

Ultra-Luminous X-ray sources are accreting black holes that might represent strong evidence of the Intermediate Mass Black Holes (IMBH), proposed to exist by theoretical studies but with no firm detection (as a class) so far. We analyze the best X-ray timing and spectral data from the ULX in NGC 5408 provided by XMM-Newton. The main goal is to study the broad-band noise variability of the source. We found an anti-correlation of the fractional root-mean square variability versus the intensity of the source, similar to black-hole binaries during hard states.

preprint2012arXivOpen access
M. D. Caballero-GarciaS. E. MottaT. M. BelloniA. Wolter
astro-ph.COastro-ph.HE
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M. D. Caballero-GarciaS. E. MottaT. M. BelloniA. Wolter

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