Accretion onto black holes and relativistic jets
Tomaso Belloni (INAF - Osservatorio Astronomico di Brera, Merate,, Italy)

TL;DR
This paper reviews recent observational advances in understanding the connection between accretion processes and relativistic jet ejections in Active Galactic Nuclei and X-ray binaries, highlighting new correlations and scaling laws.
Contribution
It provides a comprehensive review of the latest observational findings linking accretion and jet ejection in black hole systems across different scales.
Findings
Established correlations between accretion and jet ejection in X-ray binaries.
Identified scaling laws connecting AGN and X-ray binary behaviors.
Compared phenomenological properties of outbursts across systems.
Abstract
Relativistic jets from Active Galactic Nuclei are known since decades, but the study of the connection between accretion and ejection in these systems is hampered by the long time scales associated to these events. The past decade has seen a rapid advancement due to the observation of similar radio jets in galactic X-ray binaries, where the time scales are much shorter. A clear connection between accretion and ejection has been found for these systems, together with a solid characterization of the phenomenological properties of their outbursts. This wealth of new results has led to a detailed comparison between X-ray binaries and AGN, from which a number of correlations and scaling laws has been established. Here I briefly review the current observational status.
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Gamma-ray bursts and supernovae · Pulsars and Gravitational Waves Research
