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The origin and evolution of spectral curvature in blazar spectral energy distribution (SED) is still unclear. Since the observed SED curvature is related to an intrinsic curvature in emitting electron energy distribution (EED), we study…

High Energy Astrophysical Phenomena · Physics 2020-07-29 Muhammad S. Anjum , Liang Chen , Minfeng Gu

We present a high-frequency very long baseline interferometry (VLBI) kinematical study of the BL Lac object S5 0716+714 over the time period of September 2008 to October 2010. The aim of the study is to investigate the relation of the jet…

High Energy Astrophysical Phenomena · Physics 2015-06-17 B. Rani , T. P. Krichbaum , A. P. Marscher , J. A. Hodgson , L. Fuhrmann , E. Angelakis , S. Britzen , J. A. Zensus

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

Among active galactic nuclei, BL Lac objects show extreme properties that have been interpreted as the effect of relativistic beaming on the emission from a plasma jet oriented close to the line of sight. The Doppler amplification of the…

Astrophysics of Galaxies · Physics 2015-06-29 Alessandro Capetti , Claudia M. Raiteri

We are presenting a detailed parameter study of the time-dependent electron injection and kinematics and the self-consistent radiation transport in jets of intermediate and low-frequency peaked BL Lac objects. Using a time-dependent,…

Astrophysics · Physics 2009-11-07 M. Boettcher , J. Chiang

For the high-frequency peaked BL Lac object Mrk 421 we study the variation of the spectral energy distribution (SED) as a function of source activity, from quiescent to active. We use a fully automatized chi-squared minimization procedure,…

High Energy Astrophysical Phenomena · Physics 2015-05-27 Nijil Mankuzhiyil , Stefano Ansoldi , Massimo Persic , Fabrizio Tavecchio

I discuss the spectral energy distribution (SED) of all blazars with redshift detected by the {\it Fermi} satellite and listed in the 3LAC catalog. I will update the so called "blazar sequence" from the phenomenological point of view, with…

High Energy Astrophysical Phenomena · Physics 2016-09-28 Gabriele Ghisellini

The overall spectra (SED) of blazars, from radio to gamma-ray energies, seem to obey well defined trends, with a continuity of properties between blazars of different classes. To quantify this statement we can either investigate their…

Astrophysics · Physics 2007-05-23 Gabriele Ghisellini

The origin of jet launching mainly comes from two mechanisms: the BZ mechanism and the BP mechanism. However, it is in debate which one is dominating in blazars. In this work, we used a sample of 937 Fermi blazars to study the jet formation…

High Energy Astrophysical Phenomena · Physics 2024-11-19 Shangchun Xie , Zhihao Ouyang , Jingyu Wu , Hubing Xiao , Shaohua Zhang , Yongyun Chen , Zhijian Luo , Junhui Fan

Blazars host the most powerful persistent relativistic conical jet -- a highly collimated anisotropic flow of material/plasma. Motivated by this, we explore the blazar's broadband spectral energy distribution (SED) in an anisotropic flow of…

High Energy Astrophysical Phenomena · Physics 2021-06-14 Nagendra Kumar , Pankaj Kushwaha

Extreme BL Lacs (EHBL) form a subclass of blazars which challenge standard emission scenarios. In a recent study it has been argued that their peculiar properties can be explained if emitting electrons are accelerated in a series of oblique…

High Energy Astrophysical Phenomena · Physics 2022-08-03 F. Tavecchio , A. Costa , A. Sciaccaluga

In 2023 October-November, the blazar BL Lacertae underwent a very large-amplitude submm outburst. The usual single-zone leptonic model with the lower energy peak of the spectral energy distribution (SED) fit by the synchrotron emission from…

High Energy Astrophysical Phenomena · Physics 2024-11-26 Ayon Mondal , Arijit Sar , Maitreya Kundu , Ritaban Chatterjee , Pratik Majumdar

The relativistic jets produced by some Active Galactic Nuclei (AGNs) are among the most efficient persistent sources of non-thermal radiation and represent an ideal laboratory for studying high-energy interactions. In particular, when the…

High Energy Astrophysical Phenomena · Physics 2023-04-18 G. La Mura , J. Becerra Gonzalez , G. Chiaro , S. Ciroi , J. Otero-Santos

Optical light curves of bright BL Lac objects, in particular those having the SED synchrotron peak at frequencies lower than 10E14 Hz, are characterized by long-term trends with time scales of a few decades. These variations are probabily…

Astrophysics · Physics 2007-05-23 E. Massaro , F. Mantovani

The parsec-scale total intensity structures of BL Lac objects share many characteristics with quasars: e.g. well-collimated jets and superluminal motion. However, the jets of BL Lac objects appear to fade much more quickly than those in…

Astrophysics · Physics 2007-05-23 C. Reynolds , T. V. Cawthorne , D. C. Gabuzda

Relatively few Very Long Baseline Interferometry (VLBI) polarization observations have been carried out at 18 cm. The importance of such observations lies in their ability to reveal information about the jet magnetic ({\bf B}) field…

Astrophysics · Physics 2007-08-01 Péter Veres , Denise C. Gabuzda

We fit the spectral energy distributions (SEDs) of a GeV-TeV FSRQ sample with the leptonic model. Their gamma_min of the relativistic electron distributions, which significantly affect the estimates of the jet properties, are constrained,…

High Energy Astrophysical Phenomena · Physics 2014-04-29 Jin Zhang , Xiao-Na Sun , En-Wei Liang , Rui-Jing Lu , Ye Lu , Shuang-Nan Zhang

We explore the viability of the unification of BL Lacs and FR I radio galaxies by comparing the core emission of radio galaxies with those of BL Lacs, taking advantage of the newly measured optical nuclear luminosity of FR I sources. The…

Astrophysics · Physics 2007-05-23 Marco Chiaberge , Annalisa Celotti , Alessandro Capetti , Gabriele Ghisellini

We analyse a group of radio sources, a subset of the 200 mJy sample, all of which have core-jet radio structures measured with VLBI and have flat spectra stretching from the radio to the millimetre/sub-millimetre band. Thus the objects have…

Astrophysics · Physics 2009-11-10 S. Anton , I. W. A. Browne

In this review, recent progress in theoretical models for blazar emission will be summarized. The salient features of both leptonic and lepto-hadronic approaches to modeling blazar spectral energy distributions will be reviewed. I will…

High Energy Astrophysical Phenomena · Physics 2010-06-28 Markus Boettcher