Spectral/timing evolution of black-hole binaries
Tomaso M. Belloni (INAF - Osservatorio Astronomico di Brera, Merate,, Italy)

TL;DR
This paper reviews the evolution of spectral and timing properties in black-hole binaries, emphasizing the insights gained from RossiXTE observations and their implications for understanding accretion and jet ejection mechanisms.
Contribution
It summarizes the state-of-the-art paradigm of black-hole binary behavior derived from RossiXTE data and discusses its significance for accretion and jet physics.
Findings
Established the spectral/timing evolution pattern in black-hole binaries
Linked accretion processes to jet ejection phenomena
Clarified the nature of hard spectral components
Abstract
I briefly outline the state-paradigm that has emerged from the study of black-hole binaries with RossiXTE. This is the starting point of a number of studies that address the connection between accretion and jet ejection and the physical nature of the hard spectral components in these systems.
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