A spectral-timing model for ULXs in the supercritical regime
Middleton, M.J.; Heil, L.; Pintore, F.; Walton, D.J.; Roberts, T.P.
Professor Tim Roberts firstname.lastname@example.org
Ultraluminous X-ray sources (ULXs) with luminosities lying between ∼3 × 1039 and 2 × 1040 erg s−1 represent a contentious sample of objects as their brightness, together with a lack of unambiguous mass estimates for the vast majority of the central objects, leads to a degenerate scenario where the accretor could be a stellar remnant (black hole or neutron star) or intermediate-mass black hole (IMBH). Recent, high-quality observations imply that the presence of IMBHs in the majority of these objects is unlikely unless the accretion flow somehow deviates strongly from expectation based on objects with known masses. On the other hand, physically motivated models for supercritical inflows can re-create the observed X-ray spectra and their evolution, although have been lacking a robust explanation for their variability properties. In this paper, we include the effect of a partially inhomogeneous wind that imprints variability on to the X-ray emission via two distinct methods. The model is heavily dependent on both inclination to the line of sight and mass accretion rate, resulting in a series of qualitative and semiquantitative predictions. We study the time-averaged spectra and variability of a sample of well-observed ULXs, finding that the source behaviours can be explained by our model in both individual cases as well as across the entire sample, specifically in the trend of hardness-variability power. We present the covariance spectra for these sources for the first time, which shed light on the correlated variability and issues associated with modelling broad ULX spectra.
Middleton, M., Heil, L., Pintore, F., Walton, D., & Roberts, T. (2015). A spectral-timing model for ULXs in the supercritical regime. Monthly Notices of the Royal Astronomical Society, 447(4), 3243-3263. https://doi.org/10.1093/mnras/stu2644
|Journal Article Type||Article|
|Acceptance Date||Dec 12, 2014|
|Online Publication Date||Jan 16, 2015|
|Publication Date||Mar 11, 2015|
|Deposit Date||Jan 30, 2015|
|Publicly Available Date||Feb 17, 2015|
|Journal||Monthly Notices of the Royal Astronomical Society|
|Publisher||Royal Astronomical Society|
|Peer Reviewed||Peer Reviewed|
|Keywords||Accretion, Accretion discs, X-rays: binaries.|
|Related Public URLs||http://arxiv.org/abs/1412.4532|
Published Journal Article
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2015 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
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