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Related papers: Implications of Bulk Velocity Structures in AGN Je…

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BL Lacertae objects are extreme extragalactic sources characterized by the emission of strong and rapidly variable nonthermal radiation over the entire electromagnetic spectrum. Synchrotron emission followed by inverse Compton scattering in…

Astrophysics · Physics 2009-10-31 P. Giommi , G. Ghisellini , P. Padovani , G. Tagliaferri

In this review I concentrate exclusively on models for the large-scale structure created by jet flows in AGN. I briefly mention models for the evolution and emission of these objects and how they can also be applied to microquasars. While…

Astrophysics · Physics 2009-04-14 Christian R. Kaiser

Gamma-ray flares from Active Galactic Nuclei (AGN) show substantial variability on ultrafast timescales (i.e. shorter than the light crossing time of the AGN's supermassive black hole). We propose that ultrafast variability is a byproduct…

High Energy Astrophysical Phenomena · Physics 2023-04-12 Emanuele Sobacchi , Tsvi Piran , Luca Comisso

We introduce a methodology for analysis of multiwavelength data from X-ray selected BL Lac (XBL) objects detected in the TeV regime. By assuming that the radio--through--X-ray flux from XBLs is nonthermal synchrotron radiation emitted by…

Astrophysics · Physics 2009-11-13 Justin Finke , Charles Dermer , Markus Boettcher

Astrophysical jets exist in both XRBs and AGN, and seem to share common features, particularly in the radio. While AGN jets are known to emit X-rays, the situation for XRB jets is not so clear. Radio jets have been resolved in several XRBs…

Astrophysics · Physics 2009-11-07 S. Markoff , M. Nowak , S. Corbel , R. Fender , H. Falcke

Very long baseline interferometry (VLBI) observations show that some active galactic nuclei (AGN) jets exhibit bending even at parsec scales. The nature of bending is comprehensively analysed only for a small number of individual AGN, and…

High Energy Astrophysical Phenomena · Physics 2023-10-05 V. A. Makeev , Y. Y. Kovalev , A. B. Pushkarev

The spectral energy distribution and variability of several blazars (Mkn 501, 1 ES 2344+51.4, PKS 2155-30.4, 1 ES 1218+30.4, 3C 454.3) along the blazar sequence is investigated using a selfconsistent and timedependent lepto-hadronic hybrid…

High Energy Astrophysical Phenomena · Physics 2011-09-12 Matthias Weidinger , Felix Spanier

The transverse stratification of active galactic nuclei (AGN) jets is suggested by observations and theoretical arguments, as a consequence of intrinsic properties of the central engine (accretion disc + black hole) and external medium. On…

High Energy Astrophysical Phenomena · Physics 2017-10-25 O. Hervet , Z. Meliani , A. Zech , C. Boisson , V. Cayatte , C. Sauty , H. Sol

We report on the development of a numerical code to calculate the angle-dependent synchrotron + synchrotron self-Compton radiation from relativistic jet sources with partially ordered magnetic fields and anisotropic particle distributions.…

High Energy Astrophysical Phenomena · Physics 2015-06-11 Omar Jamil , Markus Boettcher

A new continuous classification system for BL Lacertae (BL Lac) objects is proposed. The peak frequency of the synchrotron component in the $\nu L_{\nu}$ spectrum is used as a classifying parameter. The application of the accelerating inner…

Astrophysics · Physics 2007-05-23 Markos Georganopoulos , Alan P. Marscher

We examine the optical properties of the nuclei of low luminosity radio-galaxies using snapshot HST images of the B2 sample. In agreement with the results obtained from the analysis of the brighter 3C/FRI sample, we find a correlation…

Astrophysics · Physics 2009-11-07 A. Capetti , A. Celotti , M. Chiaberge , H. R. de Ruiter , R. Fanti , R. Morganti , P. Parma

We compiled a sample of 24 flat-spectrum radio quasars (FSRQs), 21 BL Lacs, 13 FRI and 12 FRII radio galaxies to study the jet power and broad-line luminosity relation, and the jet power and black hole mass relation. Furthermore, we obtain…

High Energy Astrophysical Phenomena · Physics 2015-06-03 Yongyun Chen , Xiong Zhang , Haojing Zhang , Dingrong Xiong , Xiaoling Yu , Yongjuan Cha , Bijun Li , Xia Huang

The structure of Gamma-Ray Burst (GRB) jets impacts on their prompt and afterglow emission properties. Insights into the still unknown structure of GRBs can be achieved by studying how different structures impact on the luminosity function…

High Energy Astrophysical Phenomena · Physics 2015-03-05 O. S. Salafia , A. Pescalli , F. Nappo , G. Ghisellini , G. Ghirlanda , R. Salvaterra , G. Tagliaferri

The non-thermal spectra of jetted active galactic nuclei show a variety of shapes in their low- and high energy components. In some of the brightest Fermi-LAT blazars, prominent spectral breaks at a few GeV have been regularly detected,…

High Energy Astrophysical Phenomena · Physics 2016-04-20 Lars Hunger , Anita Reimer

Over 150 resolved, kpc-scale X-ray jets hosted by active galactic nuclei have been discovered with the Chandra X-ray Observatory. A significant fraction of these jets have an X-ray spectrum either too high in flux or too hard to be…

High Energy Astrophysical Phenomena · Physics 2022-12-07 Peter Breiding , Eileen T. Meyer , Markos Georganopoulos , Karthik Reddy , Kassidy E. Kollmann , Agniva Roychowdhury

Active galactic nuclei (AGN) show a range of morphologies and dynamical properties, which are determined not only by parameters intrinsic to the central engine but also their interaction with the surrounding environment. We investigate the…

High Energy Astrophysical Phenomena · Physics 2022-08-16 Soham Mandal , Paul C. Duffell , Yuan Li

The production of both gravitational waves and short gamma-ray bursts (sGRBs) is widely associated with the merger of compact objects. Several studies have modelled the evolution of the electromagnetic emission using the synchrotron…

High Energy Astrophysical Phenomena · Physics 2019-11-06 N. Fraija , D. Lopez-Camara , A. C. Caligula do E. S. Pedreira , B. Betancourt Kamenetskaia , P. Veres , S. Dichiara

We present high-quality VLA images of the FR I radio galaxy 3C 31 in the frequency range 1365 to 8440 MHz with angular resolutions from 0.25 to 40 arcsec. Our new images reveal complex, well resolved filamentary substructure in the radio…

Astrophysics · Physics 2009-11-13 R. A. Laing , A. H. Bridle , P. Parma , L. Feretti , G. Giovannini , M. Murgia , R. A. Perley

A time-dependent Synchrotron Self Compton model (SSC) which is able to motivate the used electron spectra of many SSC models as a balance of acceleration and radiative losses is introduced. Using stochastic acceleration as well as Fermi-I…

High Energy Astrophysical Phenomena · Physics 2010-08-02 Matthias Weidinger , Felix Spanier

Relativistic magnetized jets, originating near black holes, are observed to exhibit sub-structured flows. In this study, we present synthetic synchrotron emission signatures for different lines of sight and frequencies, derived from…

High Energy Astrophysical Phenomena · Physics 2024-09-25 Ravi Pratap Dubey , Christian Fendt , Bhargav Vaidya
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