| An explanation for 13 consecutive day activities of Mrk 421 |
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| 作者姓名： | Yong-Gang Zheng Chu-Yuan Yang Shi-Ju Kang Jin-Ming Bai |
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| 作者单位： | Yunnan Observatories;Department of Physics;Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment-Shandong University;Key Laboratory for the Structure and Evolution of Celestial Objects;Department of Physics and Electronics Science |
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| 基金项目： | the National Natural Science Foundation of China(Grant Nos.11673060,11763005,11873043 and 11991051);the Specialized Research Fund for Shandong Provincial Key Laboratory(Grant No.KLWH201804);the Research Foundation for Scientific Elitists of the Department of Education of Guizhou Province(Grant No.QJHKYZ[2018]068)。 |
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| 摘 要： | It is surprising to find an instance of migration in the peak positions of synchrotron spectral energy distribution components during the activity epochs of Markarian 421(Mrk 421),accompanying an orphan flare at the X-ray and GeV-TeVγ-ray bands.A geometric interpretation and standard shock or stochastic acceleration models of blazar emission have difficulty reproducing these observed behaviors.The present paper introduces a linear acceleration by integrating the reconnection electric field into the particle transport model for the observed behaviors of Mrk 421.We note that strong evidence for evolution in characteristic of multi-wavelength spectral energy distribution including shifting the peak frequency,accompanying an orphan flare at the X-ray and GeV-TeVγ-ray bands provides an important electrostatic acceleration diagnostic in a blazar jet.Assuming suitable model parameters,we apply the results of the simulation to the 13-day flaring event in March 2010 of Mrk 421,concentrating on the evolution of multiwavelength spectral energy distribution characteristic by shifting the peak frequency.It is clear that the ratio of the electric field and magnetic field strength plays an important role in temporal evolution of the peak frequency of synchrotron spectral energy distribution component.We suggest it is reasonable that the electrostatic acceleration is responsible for the evolution of multi-wavelength spectral energy distribution characteristic by shifting the peak frequency.Based on the model results,we assert that the peak frequency of the synchrotron spectral energy distribution component may signify a temporary characteristic of blazars,rather than a permanent one.
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| 关 键 词： | radiation mechanisms:non-thermal BL Lacertae objects:individual:(Mrk 421) acceleration of particles |
An explanation for 13 consecutive day activities of Mrk 421 |
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| Yong-Gang Zheng,Chu-Yuan Yang,Shi-Ju Kang,Jin-Ming Bai.An explanation for 13 consecutive day activities of Mrk 421[J].Research in Astronomy and Astrophysics,2021(1). |
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