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Related papers: Blazar Flares from Compton Dragged Shells

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We present an experimental study of the statistical properties of millimeter-size spheres floating on the surface of a turbulent flow. The flow is generated in a layer of liquid metal by an electromagnetic forcing. By using two magnet…

Fluid Dynamics · Physics 2016-07-04 Pablo Gutiérrez , Sébastien Aumaître

We have designed a new experimental setup able to investigate fracture of soft materials at small scales. At high crack velocity, where energy is mostly dissipated through viscoelastic processes, we observe an increasingly large high strain…

Soft Condensed Matter · Physics 2015-01-08 Maxime Lefranc , Elisabeth Bouchaud

We investigate experimentally the plasma dynamics of a centimeter-scale, laser filamentation-guided spark discharge. Using electrical and optical diagnostics to study monopolar discharges with varying current pulses we show that plasma…

The dissipation of turbulent magnetic fields is an appealing scenario to explain the origin of non-thermal particles in high-energy astrophysical sources. However, it has been suggested that the particle distribution may effectively…

High Energy Astrophysical Phenomena · Physics 2020-01-09 Emanuele Sobacchi , Yuri E. Lyubarsky

The multiwavelength spectra of blazars appear to be dominated by nonthermal emission from a relativistic jet oriented close to the line of sight. The recent detection of many blazars at gamma-ray energies strongly supports this scenario.…

Astrophysics · Physics 2009-10-30 C. Megan Urry

We consider the internal shock model as the dissipation mechanism responsible for the emission in blazars. It has been shown that this model is successful in reproducing the observed spectral energy distribution and the variability…

Astrophysics · Physics 2007-05-23 D. Guetta , G. Ghisellini , D. Lazzati , A. Celotti

There are still some important unanswered questions about the detailed particle acceleration and escape occurring during the quiescent epoches. As a result, the particle distribution that is adopted in the blazar quiescent spectral model…

High Energy Astrophysical Phenomena · Physics 2019-03-06 Y. G. Zheng , S. J. Kang , C. Y. Yang , J. M. Bai

A prediction for the energy shift of the synchrotron spectrum of flat-spectrum radio quasars (FSRQs) during high-energy flares is presented. If the $\gamma$-ray emission of FSRQs is produced by Comptonization of external radiation, then the…

Astrophysics · Physics 2009-10-31 M. Boettcher

Blazars exhibit flares across the electromagnetic spectrum. Many $\gamma$-ray flares are highly correlated with flares detected at optical wavelengths; however, a small subset appears to occur in isolation, with little or no variability…

High Energy Astrophysical Phenomena · Physics 2015-05-20 Nicholas R. MacDonald , Alan P. Marscher , Svetlana G. Jorstad , Manasvita Joshi

We present a detailed temporal and spectral study of the blazar 3C\,279 using multi-wavelength observations from Swift-XRT, Swift-UVOT and Fermi-LAT during a flare in 2018 January. The temporal analysis of $\gamma$-ray light curve indicates…

High Energy Astrophysical Phenomena · Physics 2021-06-03 Zahir Shah , V. Jithesh , S. Sahayanathan , Ranjeev Misra , Naseer Iqbal

Models of Blazars based on the propagation of finite discontinuities or fronts in the Poynting flux jet from the innermost regions of an accretion disk around a black hole are discussed. Such fronts may be responsible for short time-scale…

Astrophysics · Physics 2007-05-23 M. M. Romanova

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

Gamma-ray flares of blazars may be accompanied by high-energy neutrinos due to interactions of high-energy cosmic rays in the jet with photons, as suggested by the detection of the high-energy neutrino IceCube-170922A during a major…

High Energy Astrophysical Phenomena · Physics 2023-09-08 Kenji Yoshida , Maria Petropoulou , Kohta Murase , Foteini Oikonomou

We report radio imaging and monitoring observations in the frequency range 0.235 - 2.7 GHz during the flaring mode of PKS 2155-304, one of the brightest BL Lac objects. The high sensitivity GMRT observations not only reveal extended…

High Energy Astrophysical Phenomena · Physics 2016-10-19 M. Pandey-Pommier , S. Sirothia , P. Chadwick , J. -M. Martin , P. Colom , W. van Driel , F. Combes , P. Kharb , P-J. Crespeau , J. Richard , B. Guiderdoni

Recently reported coincidences between high-energy neutrino events and major blazar outbursts reinforce the relevance of lepto-hadronic emission models for blazars. We study the influence of physical parameters on the neutrino output…

High Energy Astrophysical Phenomena · Physics 2018-12-18 A. Gokus , S. Richter , F. Spanier , M. Kreter , M. Kadler , K. Mannheim , J. Wilms

We present results of variability study of a sample of 20 powerful blazars using Fermi/LAT (0.1--300 GeV) observations. We studied decade-long observations applying various analysis tools such as flux distribution, symmetry analysis, and…

High Energy Astrophysical Phenomena · Physics 2021-07-27 Gopal Bhatta , Niraj Dhital

The Fermi-LAT survey provides a large sample of blazars selected on the strength of their inverse Compton emission. We cross-correlate the first Fermi-LAT catalogue with the CRATES radio catalogue and use this sample to investigate whether…

Cosmology and Nongalactic Astrophysics · Physics 2011-06-28 J. A. Gupta , I. W. A. Browne , M. W. Peel

Context.Blazars, a sub-category of Active Galactic Nuclei, are characterized by their non-thermal variable emission. This emission extends over the whole electromagnetic spectrum and is a consequence of particle acceleration inside their…

High Energy Astrophysical Phenomena · Physics 2021-12-22 Stella S. Boula , Apostolos Mastichiadis

Blazars, a class of active galaxies whose jets are relativistic and collimated flows of plasma directed along the line of sight and are prone to a slew of magneto-hydrodynamic (MHD) instabilities. We aim to study the interplay of radiation…

High Energy Astrophysical Phenomena · Physics 2023-03-22 Sriyasriti Acharya , Bhargav Vaidya , Indu Kalpa Dihingia , Sushmita Agarwal , Amit Shukla

Bursts and flares are among the distinctive observational manifestations of magnetars, isolated neutron stars endowed with an ultra-strong magnetic field ($B \approx 10^{14}$--$10^{15}$ G). It is believed that these events arise in a hot…

High Energy Astrophysical Phenomena · Physics 2017-06-21 Roberto Taverna , Roberto Turolla