Emissive mechanism to explain spectral variability of blazars in high frequencies
文献类型：期刊论文
| 作者 | Wang JC(王建成)1,2 ; Mao JR(毛基荣)1,2
|
| 刊名 | ASTROPHYSICAL JOURNAL
 |
| 出版日期 | 2001-06-10 |
| 卷号 | 554期号:1页码:636-642 |
| 关键词 | acceleration of particles BL Lacertae objects : individual (Mrk 421) galaxies : active radiation mechanisms : nonthermal shock waves turbulence |
| ISSN号 | 0004-637X |
| 产权排序 | 第一完成单位 |
| 通讯作者 | Wang, JC (reprint author), Chinese Acad Sci, Yunnan Observ, POB 110, Kunming 650011, Yunnang Prov, Peoples R China. |
| 英文摘要 | The new results of the evolution of the synchrotron peak for Mrk 421 are mostly likely related to the particle acceleration process. In order to account for the above results, we present a model of blazar variability during the flare in which the emission comes from accelerating electrons. A diffusion advection equation of the electron energy distribution is derived to calculate the spectrum and light curve of synchrotron radiation. We present that the observed shifts of the synchrotron peak moving to higher energies during the flare are caused by shock acceleration. The observed relation between changes in the fluxes at specified frequency ranges and shifts of the peak position is fitted to constrain the physical parameters of the dissipation region. |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 学科主题 | Astronomy & Astrophysics |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | LACERTAE OBJECT PKS-2155-304 ; SELF-COMPTON MODELS ; SYNCHROTRON ; ACCELERATION |
| 收录类别 | SCI |
| 原文出处 | http://iopscience.iop.org/0004-637X/554/1/636/ |
| 语种 | 英语 |
| WOS记录号 | WOS:000169690800059 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/4934]  |
| 专题 | 云南天文台_高能天体物理研究组 |
| 作者单位 | 1.Yunnan Observatory, Chinese Academy of Sciences, P.O. Box 110, Kunming, Yunnan Province 650011, P. R. China 2.National Astronomical Observatories, Chinese Academy of Sciences and the United Laboratory of Optical Astronomy, Chinese Academy of Sciences |
| 推荐引用方式 GB/T 7714 | Wang JC,Mao JR. Emissive mechanism to explain spectral variability of blazars in high frequencies[J]. ASTROPHYSICAL JOURNAL,2001,554(1):636-642. |
| APA | Wang JC,&Mao JR.(2001).Emissive mechanism to explain spectral variability of blazars in high frequencies.ASTROPHYSICAL JOURNAL,554(1),636-642. |
| MLA | Wang JC,et al."Emissive mechanism to explain spectral variability of blazars in high frequencies".ASTROPHYSICAL JOURNAL 554.1(2001):636-642. |
入库方式： OAI收割
来源：云南天文台
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