Detection of Strong Short-Term Variability in NGC 6946 X-1
Abstract
Using two archival XMM-Newton observations, we identify strong X-ray flux variations in NGC 6946 X-1 indicating it is the most variable ultraluminous X-ray source (ULX) on mHz time scales known so far. The 1-10 keV lightcurve exhibits variability with a fractional rms amplitude of 60% integrated in the frequency range of 1-100 mHz. The power spectral density of the source shows a flat-topped spectrum that breaks at about 3 mHz with possible quasi-periodic oscillations (QPOs) near 8.5 mHz. Black hole binaries usually produce strong fast variability in the hard or intermediate state. The energy spectrum of NGC 6946 X-1 is dominated by two components, a 0.18~keV thermal disk and a power law with a photon index of ~2.2, which is consistent with the intermediate state. The characteristic time scales of the X-ray emission suggests that the ULX may contain a black hole with a mass on the order of 10^3.
Keywords
Cite
@article{arxiv.1008.2065,
title = {Detection of Strong Short-Term Variability in NGC 6946 X-1},
author = {Fengyun Rao and Hua Feng and Philip Kaaret},
journal= {arXiv preprint arXiv:1008.2065},
year = {2015}
}
Comments
5 pages, 2 figures, 2 tables. ApJ to appear