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Galactic binary systems that contain a black hole candidate emit hard X-rays in their low luminosity mode. We show that this emission can be understood as due to the Compton scattering of photons from the companion star and/or the accretion…

Astrophysics · Physics 2009-11-07 M. Georganopoulos , F. A. Aharonian , J. G. Kirk

I review recent progress in the theory of relativistic jet production, with special emphasis on unifying black hole sources of stellar and supermassive size. Observations of both classes of objects, as well as theoretical considerations,…

Astrophysics · Physics 2009-11-10 David L. Meier

The Fermi and Swift satellites, together with ground based Cherenkov telescopes, has greatly improved our knowledge of blazars, namely Flat Spectrum Radio Quasars and BL Lac objects, since all but the most powerful emit most of their…

High Energy Astrophysical Phenomena · Physics 2015-06-17 G. Ghisellini

We present a new type of observation relating the gravitational wave emission of supermassive black hole mergers to their electromagnetic counterparts. This dual emission involves variability of a relativistic jet arising from the…

High Energy Astrophysical Phenomena · Physics 2013-12-03 M. Tápai , L. Á. Gergely , Z. Keresztes , P. J. Wiita , Gopal-Krishna , P. L. Biermann

Despite the fact that jets from black holes were first understood to exist over 40 years ago, we are still in ignorance about many primary aspects of these systems -- including the radiation mechanism at high energies, the particle makeup…

High Energy Astrophysical Phenomena · Physics 2023-03-17 Eileen T. Meyer , Aamil Shaik , Karthik Reddy , Markos Georganopoulos

A jet model for Galactic black-hole X-ray binaries will be presented that appears to explain several observational characteristics. In particular, it explains the energy spectrum from radio to hard X-rays, the time-lags as a function of…

Astrophysics · Physics 2008-11-26 N. D. Kylafis , I. E. Papadakis , P. Reig

Black-hole driven relativistic astrophysical jets, such as blazars and gamma-ray bursts (GRBs), are powerful sources of electromagnetic radiation. Their emission is powered by some energy dissipation and particle acceleration mechanism…

High Energy Astrophysical Phenomena · Physics 2019-01-16 Dimitrios Giannios , Dmitri A. Uzdensky

(Abridged) We present a comprehensive study of the relation between radio and X-ray emission in neutron star X-ray binaries, use this to infer the general properties of the disc-jet coupling in such systems, and compare the results…

Astrophysics · Physics 2009-11-13 S. Migliari , R. P. Fender

There is strong observational evidence that AGN, Galactic X-ray transients and (probably) $\gamma$-ray bursts are associated with black holes, and that these sources are able to form collimated, ultrarelativistic outflows. There is much…

Astrophysics · Physics 2009-11-07 R. D. Blandford

Dense and cold clouds seem to populate the broad line region surrounding the central black hole in AGNs. These clouds could interact with the AGN jet base and this could have observational consequences. We want to study the gamma-ray…

High Energy Astrophysical Phenomena · Physics 2015-05-19 Anabella T. Araudo , Valenti Bosch-Ramon , Gustavo E. Romero

Jets are endemic to both Galactic solar mass and extragalactic supermassive black holes. A recent 86 GHz image of M\,87 shows a jet emerging from the accretion ring around a black hole, providing the first direct observational constraint on…

High Energy Astrophysical Phenomena · Physics 2024-04-22 Brian Punsly

Astrophysical jets are associated with the formation of young stars of all masses, stellar and massive black holes, and perhaps even with the formation of massive planets. Their role in the formation of planets, stars, and galaxies is…

Astrophysics · Physics 2008-08-21 Ralph E. Pudritz , Robi Banerjee , Rachid Ouyed

In outburst, neutron star X-ray binaries produce less powerful jets than black holes at a given X-ray luminosity. This has made them more difficult to study as they fade towards quiescence. To explore whether neutron stars power jets at low…

Flat radio spectra of compact jets launched by both supermassive and stellar-mass black holes are explained by an interplay of self-absorbed synchrotron emission up to some distance along the jet and optically thin synchrotron at larger…

High Energy Astrophysical Phenomena · Physics 2025-06-04 Andrzej A. Zdziarski , Callan M. Wood , Francesco Carotenuto

In this review I summarise the observational connections between accretion and relativistic outflows -- jets -- in X-ray binaries. I argue that jets are likely to be a fairly ubiquitous property of X-ray binaries as a whole, an assertion…

Astrophysics · Physics 2007-05-23 Rob Fender

Relativistic jets are one of the most powerful manifestations of the release of energy related to the supermassive black holes at the centre of active galactic nuclei (AGN). Their emission is observed across the entire electromagnetic…

High Energy Astrophysical Phenomena · Physics 2015-04-14 M. Orienti

We present a study of the mechanical power generated by both winds and jets across the black hole mass scale. We begin with the study of ionized X-ray winds and present a uniform analysis using Chandra grating spectra. The high quality…

This paper summarizes some of our recent projects which try to illuminate the nature and importance of jets associated with active nuclei and compact objects. After a short introduction on jets in radio galaxies and radio loud quasars the…

Astrophysics · Physics 2007-05-23 Heino Falcke

The black hole MAXI J1820+070 was discovered during its 2018 outburst and was extensively monitored across the electromagnetic spectrum. Following the detection of relativistic radio jets, we obtained four Chandra X-ray observations taken…

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