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The spectral properties of BL Lac objects
Wang JC(王建成); Xu J(许骏); Qian TL(钱铜铃); Cen XF(岑学奋); Wang, J
发表期刊CHINESE ASTRONOMY AND ASTROPHYSICS
1999-07
卷号23期号:3页码:288-298
DOI10.1016/S0275-1062(99)00058-2
产权排序第1完成单位
收录类别SCI
关键词Bl Lac Object Emission Mechanism Synchrotron Mechanism
摘要A model of plasma reactor is examined for a unified interpretation of the radiation of active galactic nuclei and, particularly, of BL Lac objects. The physical scenario is as follows: a large number of relativistic electrons are ejected by the central engine into the plasma reactor which surrounds the central core, and rapidly lose their energy by synchrotron radiation. Meanwhile, these electrons are accelerated by absorbing synchrotron radiation which. is not transparent in the plasma reactor and set up a steady and isotropic power law distribution with spectral index gamma=3. Then they emerge through surface diffusion or outburst of the plasma reactor and generate low-frequency synchrotron radiation. The higher frequency synchrotron radiation produced by the plasma reactor shows a rapid spectral steepening; as the flux decreases. The properties of synchrotron radiation source with radiation loss and injection of relativistic electrons are studied in detail.
语种英语
学科领域Astronomy & Astrophysics
文章类型Article
ISSN0275-1062
URL查看原文
WOS记录号WOS:000082410600006
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]LACERTAE OBJECTS ; X-RAY ; RELATIVISTIC JETS ; FAR-ULTRAVIOLET ; VARIABILITY ; BLAZARS ; RADIO ; SAMPLE ; OJ287
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文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/4927
专题高能天体物理研究组
通讯作者Wang, J
作者单位Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011 China
第一作者单位中国科学院云南天文台
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GB/T 7714
Wang JC,Xu J,Qian TL,et al. The spectral properties of BL Lac objects[J]. CHINESE ASTRONOMY AND ASTROPHYSICS,1999,23(3):288-298.
APA Wang JC,Xu J,Qian TL,Cen XF,&Wang, J.(1999).The spectral properties of BL Lac objects.CHINESE ASTRONOMY AND ASTROPHYSICS,23(3),288-298.
MLA Wang JC,et al."The spectral properties of BL Lac objects".CHINESE ASTRONOMY AND ASTROPHYSICS 23.3(1999):288-298.
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