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As part of a multi-wavelength campaign to observe the 2000--2002 outburst of the prototypical symbiotic star Z Andromedae, we observed this object six times each with the Multi-Element Radio Linked Interferometer Network (MERLIN) and Very…

Astrophysics · Physics 2009-11-10 C. Brocksopp , J. L. Sokoloski , C. Kaiser , A. M. Richards , T. W. B. Muxlow , N. Seymour

We present new [SII] images of the HH 30 jet and counterjet observed in 2006, 2007, and 2010 that allowed us to measure with improved accuracy the positions and proper motions of the jet and counterjet knots. Our results show that the…

Astrophysics of Galaxies · Physics 2015-06-05 Robert Estalella , Rosario López , Guillem Anglada , Gabriel Gómez , Angels Riera , Carlos Carrasco-González

Astrophysical jets seem to gain strength disproportionate to the power of their associated accretion flow, making low-luminosity sources ideal targets for studies of the role of outflows. Radio/X-ray correlations have supported the case for…

Astrophysics · Physics 2009-11-10 Sera Markoff

Black holes of stellar mass and neutron stars in binary systems are first detected as hard X-ray sources using high-energy space telescopes. Relativistic jets in some of these compact sources are found by means of multiwavelength…

Astrophysics · Physics 2009-10-31 I. Felix Mirabel , Luis F. Rodriguez

Black-hole and neutron-star X-ray binaries exhibit compact radio jets, when they are in the so called quiescent, hard, or hard intermediate states. The radio spectrum in these states is flat to slightly inverted. It is widely accepted that…

High Energy Astrophysical Phenomena · Physics 2017-07-26 Alexandros Tsouros , Nikolaos D. Kylafis

High-resolution Very-Long-Baseline Interferometry observations of NGC 1052 show a two sided jet with several regions of enhanced emission and a clear emission gap between the two jets.This gap shrinks with increasing frequency and vanishes…

High Energy Astrophysical Phenomena · Physics 2019-08-28 C. M. Fromm , Z. Younsi , A. Bazcko , Y. Mizuno , O. Porth , M. Perucho , H. Olivares , A. Nathanail , E. Angelakis , E. Ros , J. A. Zensus , L. Rezzolla

We demonstrate that, by combining optical, radio and X-ray observations of a Seyfert, it is possible to provide a direct measurement of the angle $\beta$ between the direction of the radio jet and the normal to the plane of the spiral host…

Some topics in the theory of jets are reviewed. These include jet precession, unconfined jets, the origin of knots, the internal shock model as a unifying theme from protostellar jets to Gamma-ray bursts, relations between the…

Astrophysics · Physics 2007-05-23 H. C. Spruit

It is widely believed that outflows of gamma-ray bursts are jetted. Some people also suggest that the jets may have structures like $\epsilon(\theta)\propto\theta^{-k}$. We test the possibility of X-ray flashes coming from such jets in this…

Astrophysics · Physics 2014-10-13 Z. P. Jin , D. M. Wei

We have investigated how varying several parameters affects the results of a collision between an extragalactic jet and a dense, intergalactic cloud, through a series of hydrodynamic simulations. We have produced synthetic radio images for…

Astrophysics · Physics 2007-05-23 Stephen Higgins , Tim O'Brien , James Dunlop

We present the theoretical background and detailed equations for the synchrotron emission of a shock wave propagating in a relativistic jet. We then show how the evolution of an outburst in this shock-in-jet scenario can be analytically…

High Energy Astrophysical Phenomena · Physics 2015-03-17 Marc Turler

We present the results of simultaneous X-ray and radio observations of the peculiar Z-type neutron star X-ray binary Cir X-1, observed with the Rossi X-ray timing explorer satellite and the Australia Telescope Compact Array in 2000 October…

High Energy Astrophysical Phenomena · Physics 2015-05-13 Paolo Soleri , Valeriu Tudose , Rob Fender , Michiel van der Klis , Peter G. Jonker

Flat radio spectra with large brightness temperatures at the core of AGN and X-ray binaries are usually interpreted as the partially self-absorbed bases of jet flows emitting synchrotron radiation. Here we extend previous models of jets…

Astrophysics · Physics 2009-11-11 Christian R. Kaiser

Seyfert galaxies and quasars were first discovered through optical and radio techniques, but in recent years high-energy emission, that can penetrate central gas and dust, has become essentially the defining characteristic of an AGN. AGNs…

Astrophysics · Physics 2007-05-23 D. M. Worrall

The collimation of a Poynting-flux dominated jet by a wind emanating from the surface of an accretion flow is computed using a semi-analytic model. The injection of the disk wind is treated as a boundary condition in the equatorial plane,…

High Energy Astrophysical Phenomena · Physics 2017-02-08 Noemie Globus , Amir Levinson

X-ray binaries are binary star systems in which a compact object (a neutron star or a black hole) and a relatively normal star orbit a common centre of mass. Since the discovery of X-ray binaries with the first X-ray telescopes in the…

Astrophysics · Physics 2008-02-07 David Russell

The extended X-ray emission observed at arcsec scales along the propagation trajectory of the precessing relativistic jets of the Galactic microquasar SS 433 features a broad emission line, with the position of the centroid being…

High Energy Astrophysical Phenomena · Physics 2017-06-28 Ildar Khabibullin , Sergey Sazonov

We review some of the ways that X-ray observations provide unique information on radio galaxies. Thermal bremsstrahlung X-ray emission provides detailed data on ambient densities and temperatures. These parameters in turn can be used for…

Astrophysics · Physics 2007-05-23 D. E. Harris

I present a brief review of the properties of jets from X-ray binaries, highlighting the disk-jet connection, in which there are strong correlations between X-ray and radio power for black holes and for neutron star in low/hard spectral…

High Energy Astrophysical Phenomena · Physics 2012-04-17 Thomas J. Maccarone

Radio observations from normal pulsars indicate that the coherent radio emission is excited by curvature radiation from charge bunches. In this review we provide a systematic description of the various observational constraints on the radio…

High Energy Astrophysical Phenomena · Physics 2024-06-03 Dipanjan Mitra , Rahul Basu , George I Melikizde
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