Parker ML, Matzeu GA, Matthews JH, Middleton MJ, Dauser T, Jiang J, Joyce A (2022)
Publication Type: Journal article
Publication year: 2022
Book Volume: 513
Pages Range: 551-572
Journal Issue: 1
Relativistic Fe K emission lines from accretion discs and from disc winds encode key information about black holes, and their accretion and feedback mechanisms. We show that these two processes can in principle produce indistinguishable line profiles, such that they cannot be disentangled spectrally. We argue that it is likely that in many cases both processes contribute to the net line profile, and their relative contributions cannot be constrained purely by Fe K spectroscopy. In almost all studies of Fe K emission to date, a single process (either disc reflection or wind Compton scattering) is assumed to dominate the total line profile. We demonstrate that fitting a single process emission model (pure reflection or pure wind) to a hybrid line profile results in large systematic biases in the estimates of key parameters, such as mass outflow rate and spin. We discuss various strategies to mitigate this effect, such as including high-energy data covering the Compton hump, and the implications for future X-ray missions.
APA:
Parker, M.L., Matzeu, G.A., Matthews, J.H., Middleton, M.J., Dauser, T., Jiang, J., & Joyce, A. (2022). The X-ray disc/wind degeneracy in AGN. Monthly Notices of the Royal Astronomical Society, 513(1), 551-572. https://doi.org/10.1093/mnras/stac877
MLA:
Parker, M. L., et al. "The X-ray disc/wind degeneracy in AGN." Monthly Notices of the Royal Astronomical Society 513.1 (2022): 551-572.
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