Interplay of spectral components in timing properties of accreting compact objects
Alexandra Veledina

TL;DR
This paper investigates how spectral components influence timing properties in accreting black hole binaries, revealing complex interactions that challenge previous models and emphasizing the importance of spectral formation conditions.
Contribution
It introduces a model considering multiple spectral components, explaining complex timing features and addressing limitations of previous propagation fluctuation models.
Findings
Phase lag amplitude becomes independent of component delays.
Power spectra can artificially decrease or increase at low frequencies.
Spectral formation conditions are crucial for understanding timing properties.
Abstract
X-ray variability of accreting black hole binaries is believed to be produced by the fluctuations propagating towards the compact object. Observations suggest the light curves in different energy bands are connected, but the fluctuations at harder energies are delayed with respect to the softer ones. The standard interpretation involves dependence of the X-ray spectral hardness on the radial distance, with harder spectra emitted closer to the black hole. Recently, a number of challenges to this scenario have been found, both at qualitative and quantitative level. The model does not predict the large magnitude of the delay between different energies, as well as the dependence of variability amplitude on the spectral range and frequency. We study timing properties of accreting black hole X-ray binaries taking into account peculiarities of spectral formation in these sources. We show that…
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