The Doppler effect and spectral energy distribution of blazars

doi:10.1088/1009-9271/1/3/213

YNAO OpenIR > 星系研究组

	The Doppler effect and spectral energy distribution of blazars
	Xie GZ(谢光中)1,2,3 ; Dai BZ(戴本忠)1,2,3 ; Mei DC(梅东成)1,2,3 ; Fan, JH4 ; Xie, GZ (reprint author), Chinese Acad Sci, Yunnan Astron Observ, Kunming 650011, Peoples R China.
发表期刊	CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS
	2001-06
卷号	1 期号:3 页码:213-220
DOI	10.1088/1009-9271/1/3/213
分类号	P158
产权排序	第1完成单位
收录类别	SCI
关键词	Blazars : General Quasars : General Radiation Mechanism : Non-thermal
摘要	The relativistic beaming model is adopted to discuss quantitatively the observational differences between radio-selected BL Lac objects (RBLs) and X-ray-selected BL Lac objects (XBLs), and between BL Lac objects and flat spectrum radio quasars (FSRQs). The main results are the following: (1) In the Doppler corrected color-color (alpha (in)(ru) - alpha (in)(ox)) diagram, XBLs and FSRQs occupy separated regions, while RBLs bridge the gap between them. These properties suggest that similar intrinsic physical processes operate in all the objects under a range of intrinsic physical conditions. (2) Our results are consistent with the results of Sambruna, Maraschi and Urry (1996) from other methods. We show the alpha (xox) introduced by Sambruna to be a good index for describing the energy distribution because it represents the intrinsic energy distribution and includes the Doppler correction. (3) The Doppler effect of relativistic beaming is the main mechanism, and the physical differences (such as magnetic fields, electron energies) are also important complementary factors for understanding the relation between XBLs and RBLs.
语种	英语
学科领域	Astronomy & Astrophysics
文章类型	Article
ISSN	1009-9271
URL	查看原文
WOS记录号	WOS:000172248900003
WOS研究方向	Astronomy & Astrophysics
WOS类目	Astronomy & Astrophysics
关键词[WOS]	BL-LACERTAE OBJECTS ; ACTIVE GALACTIC NUCLEI ; RAY-LOUD BLAZARS ; X-RAY ; COMPLETE SAMPLE ; LAC OBJECTS ; RADIO ; QUASARS ; MODEL ; POLARIZATION
引用统计	被引频次：14[WOS] [WOS记录] [WOS相关记录]
文献类型	期刊论文
条目标识符	http://ir.ynao.ac.cn/handle/114a53/6936
专题	星系研究组
通讯作者	Xie, GZ (reprint author), Chinese Acad Sci, Yunnan Astron Observ, Kunming 650011, Peoples R China.
作者单位	1.Yunnan Astronomical Observatory, Chinese Academy of Science, Kunming 650011 2.National Astronomical Observatories, Chinese Academy of Science, Beijing 100012 3.Yunnan Astrophysics Center, Yunnan University, Kunming 650091 4.Center for Astrophysics, Guangzhou Normal University, Guangzhou 510400
第一作者单位	中国科学院云南天文台
推荐引用方式 GB/T 7714	Xie GZ,Dai BZ,Mei DC,et al. The Doppler effect and spectral energy distribution of blazars[J]. CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,2001,1(3):213-220.
APA	Xie GZ,Dai BZ,Mei DC,Fan, JH,&Xie, GZ .(2001).The Doppler effect and spectral energy distribution of blazars.CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,1(3),213-220.
MLA	Xie GZ,et al."The Doppler effect and spectral energy distribution of blazars".CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS 1.3(2001):213-220.

条目包含的文件
文件名称/大小	文献类型	版本类型	开放类型	使用许可
TheDopplerEffect_省略_（383KB）	期刊论文	作者接受稿	开放获取	CC BY-NC-SA	浏览请求全文