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
DOI10.1088/1009-9271/1/3/213
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
ISSN1009-9271
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
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
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
个性服务
推荐该条目
保存到收藏夹
查看访问统计
导出为Endnote文件
谷歌学术
谷歌学术中相似的文章
[Xie GZ(谢光中)]的文章
[Dai BZ(戴本忠)]的文章
[Mei DC(梅东成)]的文章
百度学术
百度学术中相似的文章
[Xie GZ(谢光中)]的文章
[Dai BZ(戴本忠)]的文章
[Mei DC(梅东成)]的文章
必应学术
必应学术中相似的文章
[Xie GZ(谢光中)]的文章
[Dai BZ(戴本忠)]的文章
[Mei DC(梅东成)]的文章
相关权益政策
暂无数据
收藏/分享
文件名: TheDopplerEffect_省略_ibutionofBlazars_.pdf
格式: Adobe PDF
所有评论 (0)
暂无评论
 

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。