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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

We report on the variations of the physical parameters of the jet observed in the blazar Mrk 421, and discuss the origin of X-ray flares in the jet, based on the analysis of the several spectral energy distributions (SEDs). The SEDs are…

High Energy Astrophysical Phenomena · Physics 2020-05-27 Yurika Yamada , Makoto Uemura , Ryosuke Itoh , Yasushi Fukazawa , Masanori Ohno , Fumiya Imazato

For the first time, Kataoka \& Stawarz reported a clear detection of a hard X-ray excess, above $\gtrsim$20 keV, in the high-synchrotron-peaked BL Lac object Mrk 421. We find that this feature may not be produced by the low-energy part of…

High Energy Astrophysical Phenomena · Physics 2017-07-27 Liang Chen

Due to its proximity, Markarian 421 is one of the most extensively studied jetted active galactic nuclei. Its spectral energy distribution and light curve are widely studied, serving as primary means for understanding jet radiation…

High Energy Astrophysical Phenomena · Physics 2025-07-03 Rui Xue , Ze-Rui Wang , Hai-Bin Hu

We present the timing analysis of 10 archived \XMM observations with an exposure of $>40$ ks of Markarian 421. Mrk 421 is the brightest high-frequency-peaked BL Lac object (HBL) emitting in X-rays produced by electrons accelerated in the…

High Energy Astrophysical Phenomena · Physics 2024-06-25 Wen Hu , Jia-Lai Kang , Zhen-Yi Cai , Jun-Xian Wang , Zhen-Bo Su , Guang-Cheng Xiao

By fitting high-quality and simultaneous multi-wavelength (MWL) spectral energy distributions (SEDs) at multiple epochs with a one-zone leptonic jet model, we study jet properties of the three famous blazars Mrk 421, 3C 454.3 and 3C 279. In…

High Energy Astrophysical Phenomena · Physics 2021-04-07 Wen Hu , Da-hai Yan , Qiang-lin Hu

We investigate the X-ray and $\gamma$-ray flares of Mrk 421 on 2008 June 6-15 using the synchrotron self- Compton(SSC) model with electron acceleration, in which an evident correlation between the X-ray and $\gamma$-ray bands appears, while…

High Energy Astrophysical Phenomena · Physics 2015-06-16 Gang Cao , Jiancheng Wang

It is well known that the flat radio spectrum is a common property in the spectral energy distribution of blazars. Although the one-zone leptonic models are generally successful in explaining the multi-wave band emission, they are…

High Energy Astrophysical Phenomena · Physics 2021-06-02 Rui Xue , Ze-Rui Wang

It is surprising to find a fact for migration in the peak positions of synchrotron spectra energy distribution component during in the activity epochs of Mrk 421, accompanying with an orphan flaring at the X-ray and GeV-TeV $\gamma$-ray…

High Energy Astrophysical Phenomena · Physics 2021-02-10 Y. G. Zheng , C. Y. Yang , Shi-Ju Kang , J. M. Bai

The availability of simultaneous X-ray and Very High Energy (VHE) observations of blazars helps to identify the plausible radiative contributors to the VHE emission. Under leptonic scenario, the VHE emission from BL Lacs are attributed to…

High Energy Astrophysical Phenomena · Physics 2023-08-21 Aaqib Manzoor , Sunder Sahayanathan , Zahir Shah , Subir Bhattacharyya , Naseer Iqbal , Zahoor Malik

We examine the applicability of the stochastic electron acceleration to two high synchrotron peaked blazars, Mrk 421 and Mrk 501, assuming synchrotron self-Compton emission of gamma-rays. Our model considers an emitting region moving at…

High Energy Astrophysical Phenomena · Physics 2015-06-23 Jun Kakuwa , Kenji Toma , Katsuaki Asano , Masaaki Kusunose , Fumio Takahara

There is an increasing number of observational evidence that very high energy gamma-rays in radio-loud active galactic nuclei are produced in the direct vicinity of a supermassive black hole (SMBH), close to the base of a relativistic jet.…

High Energy Astrophysical Phenomena · Physics 2022-11-30 Piotr Banasinski , Wlodek Bednarek

We report on the findings of a 364 ksec observation of the BL LAC object Mrk 421 with the X-ray observatory Suzaku. The analysis in this paper uses fluxes and hardness ratios in the broad energy range from 0.5 keV to 30 keV. During the…

High Energy Astrophysical Phenomena · Physics 2015-05-19 Alfred B. Garson , Matthew G. Baring , Henric Krawczynski

We present the results of extensive modeling of the spectral energy distributions (SEDs) of the closest blazar (z=0.031) Markarian 421 (Mrk 421) during a giant outburst in February 2010. The source underwent rapid flux variations in both…

Astrophysics of Galaxies · Physics 2019-05-29 B. Banerjee , M. Joshi , P. Majumdar , K. E. Williamson , S. G. Jorstad , A. P. Marscher

Strong X-ray and $\gamma$--ray flares have been detected in February 2010 from the high synchrotron peaked blazar Mrk 421 (z=0.031). With the motivation of understanding the physics involved in this flaring activity, we study the…

(abridged) We present a new time-dependent multi-zone radiative transfer code and its application to study the SSC emission of Mrk 421. The code couples Fokker-Planck and Monte Carlo methods, in a 2D geometry. For the first time all the…

High Energy Astrophysical Phenomena · Physics 2011-09-22 Xuhui Chen , Giovanni Fossati , Edison Liang , Markus Boettcher

A hard TeV $\gamma$-ray component excess over the single-zone leptonic model prediction (TeV excess) is observed in the spectral energy distributions (SEDs) of some BL Lacs. Its origin is uncertain. We revisit this issue with four BL Lacs…

High Energy Astrophysical Phenomena · Physics 2022-02-09 Ji-Gui Cheng , Xiao-Li Huang , Ze-Rui Wang , Jian-Kun Huang , En-Wei Liang

During the observation period 1997, the nearby Blazar Mkn 501 showed extremely strong emission and high variability. We examine multiwavelength aspects of this event using radio, optical, soft and hard X-ray and TeV data. We concentrate on…

Multiwavelength variability of blazars offers indirect insight into their powerful engines and on the mechanisms through which energy is propagated from the centre down the jet. The BL Lac object Mkn 421 is a TeV emitter, a bright blazar at…

Mkn 421 is a nearby active galactic nucleus dominated at all wavelengths by a very broad non-thermal continuum thought to arise from a relativistic jet seen at a small angle to the line of sight. Its spectral energy distribution peaks in…

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