Optical spectroscopy of four young radio sources
文献类型:期刊论文
作者 | Fan, XL; Bai, JM; Hu, C![]() ![]() |
刊名 | NEW ASTRONOMY
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出版日期 | 2017 |
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 |
DOI | 10.1016/j.newast.2016.07.009 |
文献子类 | Article |
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. |
电子版国际标准刊号 | 1384-1092 |
WOS关键词 | ACTIVE GALACTIC NUCLEI ; SEYFERT 1 GALAXIES ; BLACK-HOLE MASSES ; LUMINOSITY COMPACT SOURCES ; EDDINGTON RATIO ; STEEP-SPECTRUM ; EMISSION-LINE ; LOUD ; EVOLUTION ; QUASARS |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
WOS记录号 | WOS:000384387500011 |
源URL | [http://ir.ihep.ac.cn/handle/311005/284302] ![]() |
专题 | 高能物理研究所_粒子天体物理中心 |
作者单位 | 中国科学院高能物理研究所 |
推荐引用方式 GB/T 7714 | Fan, XL,Bai, JM,Hu, C,et al. Optical spectroscopy of four young radio sources[J]. NEW ASTRONOMY,2017,50:78-81. |
APA | Fan, XL,Bai, JM,Hu, C,Wang, JG,&胡晨.(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:高能物理研究所
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