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- W2149107030 abstract "Aims. Both the well known microquasar GRS 1915+105, as well as its recently discovered analogue, IGR J17091-3624, exhibit variability that is characteristic of a deterministic chaotic system. Their specific kind of quasi-periodic flares that are observed in some states is intrinsically connected with the global structure of the accretion flow, which are governed by the nonlinear hydrodynamics. One plausible mechanism that is proposed to explain this kind of variability is the thermal-viscous instability that operates in the accretion disk. The purely stochastic variability that occurs because of turbulent conditions in the plasma, is quantified by the power density spectra and appears in practically all types of sources and their spectral states." @default.
- W2149107030 created "2016-06-24" @default.
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- W2149107030 date "2016-02-01" @default.
- W2149107030 modified "2023-10-17" @default.
- W2149107030 title "Chaotic and stochastic processes in the accretion flows of the black hole X-ray binaries revealed by recurrence analysis" @default.
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- W2149107030 doi "https://doi.org/10.1051/0004-6361/201526692" @default.
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