Optical spectroscopy of four young radio sources
文献类型：期刊论文
| 作者 | Fan XL(范绪亮)1,2,4 ; Bai JM(白金明)1,2; Hu, Chen3; Wang JG(王建国)1,2
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| 刊名 | NEW ASTRONOMY
 |
| 出版日期 | 2017-01 |
| 卷号 | 50页码:78-81 |
| 关键词 | Galaxies: jets quasars: emission lines quasars: individual (GB6 J0140+4024 TXS 0942+355 IRAS 11119+3257 4C 12.50) |
| ISSN号 | 1384-1076 |
| 产权排序 | 第一完成单位 |
| 通讯作者 | Fan, XL |
| 英文摘要 | We report the optical spectroscopy of four young radio sources which are observed with the Lijiang 2.4 m telescope. The Eddington ratios of these sources are similar with those of narrow-line Seyfert 1 galaxies (NLS1s). Their Fe II emission is strong while [O III] strength is weak. These results confirm the NLS1 features of young radio sources, except that the width of broad H beta of young radio sources is larger than that of NLS1s. We thus suggest that the young radio sources are the high black hole mass counterparts of steep-spectrum radio-loud NLS1s. In addition, the broad H beta component of 4C 12.50 is the blue wing of the narrow component, but not from the broad line region. (C) 2016 Elsevier B.V. All rights reserved. |
| 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 ; SEYFERT 1 GALAXIES ; BLACK-HOLE MASSES ; LUMINOSITY COMPACT SOURCES ; EDDINGTON RATIO ; STEEP-SPECTRUM ; EMISSION-LINE ; LOUD ; EVOLUTION ; QUASARS |
| 收录类别 | SCI |
| 原文出处 | http://www.sciencedirect.com/science/article/pii/S1384107616300537 |
| 语种 | 英语 |
| WOS记录号 | WOS:000384387500011 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/9723]  |
| 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 650011, China 2.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650011, China 3.Key Laboratory for Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, 19B Yuquan Road,Beijing 100049, China 4.University of Chinese Academy of Sciences, Beijing 100049, China |
| 推荐引用方式 GB/T 7714 | Fan XL,Bai JM,Hu, Chen,et al. Optical spectroscopy of four young radio sources[J]. NEW ASTRONOMY,2017,50:78-81. |
| APA | Fan XL,Bai JM,Hu, Chen,&Wang JG.(2017).Optical spectroscopy of four young radio sources.NEW ASTRONOMY,50,78-81. |
| MLA | Fan XL,et al."Optical spectroscopy of four young radio sources".NEW ASTRONOMY 50(2017):78-81. |
入库方式： OAI收割
来源：云南天文台
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