The Doppler effect and spectral energy distribution of blazars
文献类型：期刊论文
| 作者 | 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
|
| 刊名 | CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS
 |
| 出版日期 | 2001-06 |
| 卷号 | 1期号:3页码:213-220 |
| 关键词 | blazars : general quasars : general radiation mechanism : non-thermal |
| ISSN号 | 1009-9271 |
| 产权排序 | 第一完成单位 |
| 通讯作者 | Xie, GZ (reprint author), Chinese Acad Sci, Yunnan Astron Observ, Kunming 650011, Peoples R China. |
| 英文摘要 | 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. |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 学科主题 | Astronomy & Astrophysics |
| 分类号 | P158 |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | 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 |
| 收录类别 | SCI |
| 原文出处 | http://iopscience.iop.org/1009-9271/1/3/213/ |
| 语种 | 英语 |
| WOS记录号 | WOS:000172248900003 |
| 公开日期 | 2016-05-03 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/6936]  |
| 专题 | 云南天文台_星系研究组 |
| 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.(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. |
入库方式： OAI收割
来源：云南天文台
浏览0
下载0
收藏0
其他版本
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。