HINTS OF CORRELATION BETWEEN BROAD-LINE AND RADIO VARIATIONS FOR 3C 120
文献类型:期刊论文
作者 | Liu HT(刘洪涛)1,2![]() ![]() ![]() ![]() |
刊名 | ASTRONOMICAL JOURNAL
![]() |
出版日期 | 2014-01 |
卷号 | 147期号:1页码:17- |
关键词 | galaxies: active galaxies: individual (3C 120) galaxies: jets quasars: emission lines radio continuum: galaxies |
ISSN号 | 0004-6256 |
产权排序 | 第一完成单位 |
通讯作者 | Liu, HT (reprint author), Chinese Acad Sci, Yunnan Observ, Kunming 650011, Yunnan, Peoples R China. |
英文摘要 | In this paper, we investigate the correlation between broad-line and radio variations for the broad-line radio galaxy 3C 120. By the z-transformed discrete correlation function method and the model-independent flux randomization/random subset selection (FR/RSS) Monte Carlo method, we find that broad H beta line variations lead the 15 GHz variations. The FR/RSS method shows that the H beta line variations lead the radio variations by a factor of tau(ob) = 0.34 +/- 0.01 yr. This time lag can be used to locate the position of the emitting region of radio outbursts in the jet, on the order of similar to 5 lt-yr from the central engine. This distance is much larger than the size of the broad-line region. The large separation of the radio outburst emitting region from the broad-line region will observably influence the gamma-ray emission in 3C 120. |
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] | ACTIVE GALACTIC NUCLEI ; GAMMA-RAY EMISSION ; HIGH-ENERGY EMISSION ; SEYFERT 1 GALAXIES ; OPTICAL CONTINUUM ; LOUD QUASARS ; OBSERVATIONAL EVIDENCE ; RELATIVISTIC JET ; ACCRETION-DISK ; EXTENDED RADIO |
收录类别 | SCI |
原文出处 | http://iopscience.iop.org/article/10.1088/0004-6256/147/1/17/meta |
语种 | 英语 |
WOS记录号 | WOS:000328694500017 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/5453] ![]() |
专题 | 云南天文台_丽江天文观测站(南方基地) 云南天文台_中国科学院天体结构与演化重点实验室 |
作者单位 | 1.Yunnan Observatories, Chinese Academy of Sciences, Kunming, Yunnan 650011, China 2.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming, Yunnan 650011, China 3.Key Laboratory for Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, 19B Yuquan Road, Beijing 100049, China 4.Theoretical Physics Center for Science Facilities, Chinese Academy of Sciences, Beijing 100049, China |
推荐引用方式 GB/T 7714 | Liu HT,Bai JM,Wang, JM,et al. HINTS OF CORRELATION BETWEEN BROAD-LINE AND RADIO VARIATIONS FOR 3C 120[J]. ASTRONOMICAL JOURNAL,2014,147(1):17-. |
APA | Liu HT,Bai JM,Wang, JM,&Li SK.(2014).HINTS OF CORRELATION BETWEEN BROAD-LINE AND RADIO VARIATIONS FOR 3C 120.ASTRONOMICAL JOURNAL,147(1),17-. |
MLA | Liu HT,et al."HINTS OF CORRELATION BETWEEN BROAD-LINE AND RADIO VARIATIONS FOR 3C 120".ASTRONOMICAL JOURNAL 147.1(2014):17-. |
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。