An explanation about the flat radio spectrum for Mrk 421

• 作者: Rui Xue Ze-Rui Wang
• 来源期刊: 天文和天体物理学研究
• 年，卷（期）: 2021,（4）
• 页码范围: 233-240
• 页数: 8页
• 语种: 英文
• DOI: 10.1088/1674-4527/21/4/103

摘要

It is well known that a fiat radio spectrum is a common property in the spectral energy distribution of blazars.Although one-zone leptonic models are generally successful in explaining the multi-wave band emission,they are problematic in reproducing the radio spectrum.In the study of Mrk 421,one-zone models suggest that in order to avoid overproducing the radio flux,the minimum electron Lorentz factor should be larger than a few hundred at least,even considering the synchrotron self-absorption effect.This result suggests that the model predicted spectral index in the radio band of Mrk 421 should be-1/3.On the basis of this result,by assuming there is a neglected region that will also contribute the radio emission and its electron energy index naturally originates from the simplest first-order Fermi acceleration mechanism,we can get a superimposed flat radio spectrum.In this paper,a two-zone model is proposed to reproduce the quiescent state spectral energy distribution of Mrk 421.In addition to taking into account the emission from a conventional radiation zone,we further consider emission from the acceleration zone in which particles are accelerated at a shock front.With the present model,our fitting result suggests that the low frequency fiat radio spectrum of Mrk 421 might be explained as a superposition of the synchrotron emission from acceleration zone and radiation zone.