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Related papers: On The Jets Associated with Galactic Superluminal …

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High energy emission can be produced in the interaction sites of both galactic and extragalactic jets with the surrounding medium. We have developed a radiative model that accounts for the continuous injection of relativistic electrons in…

High Energy Astrophysical Phenomena · Physics 2011-07-14 P. Bordas , V. Bosch-Ramon , M. Perucho

GeV-TeV gamma-ray and PeV-EeV neutrino backgrounds provide a unique window on the nature of the ultra-high-energy cosmic-rays (UHECRs). We discuss the implications of the recent Fermi-LAT data regarding the extragalactic gamma-ray…

High Energy Astrophysical Phenomena · Physics 2017-07-06 Noemie Globus , Denis Allard , Etienne Parizot , Tsvi Piran

We obtain the maximum diffuse neutrino intensity predicted by hadronic photoproduction models of the type which have been applied to the jets of active galactic nuclei or gamma ray bursts. For this, we compare the proton and gamma ray…

Astrophysics · Physics 2010-12-03 K. Mannheim , R. J. Protheroe , J. P. Rachen

A puzzling feature of the {\it Chandra}--detected quasar jets is that their X-ray emission decreases faster along the jet than their radio emission, resulting to an outward increasing radio to X-ray ratio. In some sources this behavior is…

Astrophysics · Physics 2016-08-30 Markos Georganopoulos , Demosthenes Kazanas

I discuss the spectral features of pi-0 decay gamma-radiation from clouds/targets located in proximity of relatively young proton accelerators, and speculate that such ``accelerator+target'' systems in our Galaxy can be responsible for a…

Astrophysics · Physics 2021-04-28 F. A. Aharonian

It is shown that the two-sided jet proper motions observed from the galactic microquasars GRS 1915+105 and GRO J1655-40 in practice only allow us to place lower limits on the Lorentz factors of the outflows. As a consequence, it is not…

Astrophysics · Physics 2009-11-07 R. P. Fender

We examine a systematic comparison of jet-knots, hotspots and radio lobes recently observed with Chandra and ASCA. This report will discuss the origin of their X-ray emissions and investigate the dynamics of the jets. The data was compiled…

Astrophysics · Physics 2009-11-10 Jun Kataoka , Lukasz Stawarz

The connection between the arrival directions of ultrahigh energy cosmic rays by using the EAS array data and point galactic sources of radio-and gamma-radiations, pulsars,is sought. At the mean particle energy of 10^{19} eV the correlation…

Astrophysics · Physics 2007-05-23 A. A. Mikhailov

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

A list is presented of known extragalactic radio jets which also have associated X-ray emission. The canonical emission processes for the production of X-rays are reviewed and the sources are categorized on the basis of our current…

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

Gamma rays trace accelerated particles, and the observed flux of extragalactic gamma rays therefore constrains the global efficiency for particle acceleration. Extragalactic jets in active galactic nuclei can account for the gamma ray…

Astrophysics · Physics 2014-10-13 Karl Mannheim

Context. The microquasar 1E 1740.7-2942 is a source located in the direction of the Galactic Center. It has been detected at X-rays, soft gamma-rays, and in the radio band, showing an extended radio component in the form of a double-sided…

Astrophysics · Physics 2009-11-11 V. Bosch-Ramon , G. E. Romero , J. M. Paredes , A. Bazzano , M. Del Santo , L. Bassani

The X-ray/radio transient superluminal jet source GRO J1655-40 was recently suggested to contain a black hole from optical observations. Being a relatively close-by system (d \sim 3.2 kpc), it can likely provide us with rich information…

The EGRET catalogue of unidentified X-ray sources has more objects along the galactic disk than at high galactic latitude, where identifications are comparatively easier. On the other hand, the Egret/GRO mission has already identified…

Astrophysics · Physics 2009-10-30 P. A. Caraveo , G. F. Bignami

A subset of the unidentified EGRET gamma-ray sources with no active galactic nucleus or other conspicuous counterpart appears to be concentrated at medium latitudes. Their long-term variability and their spatial distribution indicate that…

Astrophysics · Physics 2009-11-10 I. A. Grenier , M. M. Kaufman Bernado , G. E. Romero

The cosmic ray source spectrum produced by AGN (Active Galactic Nucleus) jets is calculated. A distinctive feature of these calculations is the account for the jet distribution on kinetic energy. The expected cosmic ray spectrum at the…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-28 V. S. Ptuskin , S. I. Rogovaya , V. N. Zirakashvili

We investigate the association between the radio ``plateau'' states and the large superluminal flares in GRS 1915+105 and propose a qualitative scenario to explain this association. We identify several candidate superluminal flare events…

This review provides the background and current perspective of some of the striking asymmetries exhibited by extragalactic double-lobed radio sources, paying special attention to the reported interrelationships among some of them. We…

Astrophysics · Physics 2007-05-23 Gopal-Krishna , Paul J. Wiita

Here we discuss evolution and broad-band emission of compact (< kpc) lobes in young radio sources. We propose a simple dynamical description for these objects, consisting of a relativistic jet propagating into a uniform gaseous medium in…

Astrophysics · Physics 2009-11-13 L. Stawarz , L. Ostorero , M. C. Begelman , R. Moderski , J. Kataoka , S. Wagner

Very high energy (VHE) gamma-rays from extragalactic sources, interacting by gamma-gamma collisions with diffuse intergalactic radiation fields, provide an alternative way to constrain the diffuse background light, completely independent of…

High Energy Astrophysical Phenomena · Physics 2015-06-04 Luigi Costamante
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