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Related papers: Decomposing blazar spectra into lepto-hadronic emi…

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We investigate the origin of high-energy emission in blazars within the context of the leptohadronic one-zone model. We find that $\gamma$-ray emission can be attributed to synchrotron radiation either from protons or from secondary leptons…

High Energy Astrophysical Phenomena · Physics 2015-06-15 Apostolos Mastichiadis , Maria Petropoulou , Stavros Dimitrakoudis

The measured spectral energy distribution and variability time scale are used to determine the radiation and magnetic-field energy densities in the relativistic plasma that forms the gamma-ray emitting jet in the blazar 3C 279. Assuming…

Astrophysics · Physics 2007-05-23 C. D. Dermer , A. Atoyan

The evidence for joint gamma and neutrino emission from the blazar TXS 0506+056 has renewed interest in blazars as neutrino sources. The detection of neutrinos from blazars can be seen as the smoking gun for the presence of relativistic…

High Energy Astrophysical Phenomena · Physics 2020-05-20 Matteo Cerruti

The origin of high-energy emission in blazars jets (i.e., leptonic versus hadronic) has been a long-standing matter of debate. Here, we focus on one variant of hadronic models where proton synchrotron radiation accounts for the observed…

High Energy Astrophysical Phenomena · Physics 2020-04-28 I. Liodakis , M. Petropoulou

The high-peaked BL Lac object Pks2155-304 shows high variability at multiwavelengths, i.e. from optical up to TeV energies. A giant flare of around 1 hour at X-ray and TeV energies was observed in 2006. In this context, it is essential to…

High Energy Astrophysical Phenomena · Physics 2016-05-25 Julia K. Becker , Athina Meli , Peter L. Biermann

The observation of IceCube-170922A event from the direction of TXS 0506+056 when it was in its enhanced $\gamma$-ray emission state offers a unique opportunity to investigate the lepto-hadronic processes in blazar jets. Here, the observed…

High Energy Astrophysical Phenomena · Physics 2018-10-24 N. Sahakyan

Blazars are a subclass of active galactic nuclei (AGN) that have a relativistic jet with a small viewing angle towards the observer. Recent results based on hadronic scenarios have motivated an ongoing discussion of how a blazar can produce…

High Energy Astrophysical Phenomena · Physics 2021-01-07 A. Rosales de León , A. M. Brown , P. M. Chadwick

Recent observations are shedding light on the important role that active galactic nuclei (AGN) play in the production of high-energy neutrinos. In this study, we focus on one object, 5BZB J0630-2406, which is among the blazars recently…

The emission of the so-called extreme blazars challenges the particle acceleration models. The hardness of its spectrum, $<2$, demands extreme parameters using the standard one-zone SSC model in the high energy band. Some authors use both…

High Energy Astrophysical Phenomena · Physics 2021-08-27 E. Aguilar-Ruiz , N. Fraija

Blazars are the most violent steady/recurrent sources of high-energy gamma-ray emission in the known Universe. They are prominent emitters of electromagnetic radiation throughout the entire electromagnetic spectrum. The observable radiation…

Astrophysics · Physics 2008-11-26 Markus Boettcher

Various aspects of the high-energy emission from relativistic jets associated wi th compact astrophysical systems are reviewed. The main leptonic and hadronic processes responsible for the production of high-energy $\gamma$-rays, very-high…

Astrophysics · Physics 2008-11-26 Amir Levinson

Blazars have been suggested as possible neutrino sources long before the recent IceCube discovery of high-energy neutrinos. We re-examine this possibility within a new framework built upon the blazar simplified view and a self-consistent…

High Energy Astrophysical Phenomena · Physics 2015-08-06 P. Padovani , M. Petropoulou , P. Giommi , E. Resconi

The blazar $TXS~0506+056$ has been proposed as a high-energy neutrino emitter. However, it has been shown that the standard one-zone model cannot produce sufficiently high neutrino flux due to constraints from the X-ray data, implying more…

High Energy Astrophysical Phenomena · Physics 2024-01-19 Zhen-Jie Wang , Ruo-Yu Liu , Ze-Rui Wang , Junfeng Wang

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

Recent observations of VER J2227+608 reveal a broken power $\gamma$-ray spectrum with the spectral index increasing from $\sim 1.8$ in the GeV energy range to $\sim 2.3$ in the TeV range. Such a spectral break can be attributed to radiative…

High Energy Astrophysical Phenomena · Physics 2020-07-22 Siming Liu , Houdun Zeng , Yuliang Xin , Hui Zhu

The interest in blazars as candidate neutrino emitters grew after the 3$\sigma$ evidence for a contemporaneous joint photon and neutrino emission from the flaring blazar TXS 0506+056 in 2017. Blazars, a class of extragalactic sources with…

High Energy Astrophysical Phenomena · Physics 2025-11-27 Ilaria Viale , Giacomo Principe , Chiara Righi , Matteo Cerruti , Fabrizio Tavecchio , Elisa Bernardini

In this work we investigate the nature of multi-wavelength variability of blazars from a purely numerical approach. We use a time-dependent one-zone leptonic blazar emission model to simulate multi-wavelength variability by introducing…

High Energy Astrophysical Phenomena · Physics 2022-02-09 Hannes Thiersen , Michael Zacharias , Markus Böttcher

We present a general self-consistent lepto/hadronic jet model for the non-thermal electromagnetic emission of microquasars. The model is applied to the low-mass microquasar (LMMQ) GX 339-4 and predicts its high-energy features. We assume…

High Energy Astrophysical Phenomena · Physics 2015-05-14 Gabriela S. Vila , Gustavo E. Romero

The jets of blazars are renowned for their multi-wavelength flares and rapid extreme variability; however, there are still some important unanswered questions about the physical processes responsible for these spectral and temporal changes…

High Energy Astrophysical Phenomena · Physics 2020-10-30 Y. G. Zheng , S. J. Kang , C. Y. Yang , J. M. Bai

We examine the neutrino and cosmic ray spectra resulting from two models of fitting the spectral energy distribution (SED) of the blazar Mrk~421 using a self-consistent leptohadronic code. The $\gamma$-ray emission is attributed to either…

High Energy Astrophysical Phenomena · Physics 2015-06-17 Stavros Dimitrakoudis , Maria Petropoulou , Apostolos Mastichiadis