中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Supermassive Black Holes with High Accretion Rates in Active Galactic Nuclei. XV. Reverberation Mapping of Mg ii Emission Lines

文献类型:期刊论文

作者Bai, Hua-Rui11,12; Du, Pu11; Hu, Chen11; Chen, Yong-Jie11,13; Yao, Zhu-Heng1,14; Li, Yan-Rong11; Fu, Yi-Xin11,12; Wang, Yi-Lin11,12; Zhao, Yu11,12; Zhang, Hao11,12
刊名ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
出版日期2026-02-01
卷号282期号:2
ISSN号0067-0049
DOI10.3847/1538-4365/ae2b6d
产权排序第8完成单位
文献子类Article
英文摘要As the 15th paper in a series reporting on a large reverberation mapping (RM) campaign of super-Eddington accreting massive black holes (SEAMBHs) in active galactic nuclei (AGNs), we present the results of measurements of the Mg ii lines in 18 SEAMBHs monitored spectroscopically from 2017 to 2024. Among these, the time lags of Mg ii have been successfully determined for eight of the 18 objects, thereby expanding the current Mg ii RM sample, particularly at higher accretion rates. By incorporating measurements of the line widths, we determine the masses of their central supermassive black holes. Based on these new measurements, we update the relation between the Mg ii radius and the monochromatic luminosity at 3000 & Aring; (RMgII-L3000 relation), yielding a slope of 0.24 +/- 0.03, which is slightly shallower than, yet still consistent with, previously reported values. Similar to the H beta lines, the Mg ii time lags in SEAMBHs are shorter than those of AGNs with normal accretion rates at comparable luminosities. The deviation of AGNs from the best-fit RMgII-L3000 relation shows a strong correlation with the accretion rate, while no significant correlation is found between the deviation and the flux ratio of UV iron to Mg ii.
学科主题天文学 ; 天体物理学 ; 高能天体物理学 ; 星系与宇宙学
URL标识查看原文
出版地No.2 The Distillery, Glassfields, Avon Street, Bristol, ENGLAND
WOS关键词RADIUS-LUMINOSITY RELATION ; TIME-DELAY MEASUREMENT ; OPTICAL FE II ; H-BETA ; MASS ESTIMATORS ; EDDINGTON RATIO ; INTERMEDIATE-REDSHIFT ; SPECTRAL VARIABILITY ; CTS C30.10 ; FLUX RATIO
资助项目National Key R&D Program of China[2021YFA1600404]; MOST divided by NSFC divided by Key Programme[12333003]; China Manned Space Project[CMS-CSST-2025-A07]; National Science and Technology Major Project[2024ZD0300303]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001674903400001
出版者IOP Publishing Ltd
资助机构National Key R&D Program of China[2021YFA1600404] ; MOST divided by NSFC divided by Key Programme[12333003] ; China Manned Space Project[CMS-CSST-2025-A07] ; National Science and Technology Major Project[2024ZD0300303]
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/28897]  
专题云南天文台_丽江天文观测站(南方基地)
通讯作者Du, Pu
作者单位1.Key Laboratory of Space Astronomy and Technology, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, People’s Republic of China;
2.College of Physics and Electrical Engineering, Anyang Normal University, Anyang, Henan 455000, People’s Republic of China;
3.School of Astronomy and Space Sciences, University of Chinese Academy of Sciences, Beijing 100049, People’s Republic of China
4.Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, People’s Republic of China;
5.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, People’s Republic of China;
6.College of Physics and Information Engineering, Quanzhou Normal University, Quanzhou, Fujian 362000, People’s Republic of China;
7.Centro Astronomico Hispano Alemán, Sierra de los Filabres sn, E-04550 Gergal, Almería, Spain;
8.Instituto de Astrofísica de Andalucía (CSIC), Glorieta de la Astronomía sn, E-18008 Granada, Spain;
9.Department of Astronomy, School of Physics, Peking University, Beijing 100871, People’s Republic of China;
10.The Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, People’s Republic of China;
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GB/T 7714
Bai, Hua-Rui,Du, Pu,Hu, Chen,et al. Supermassive Black Holes with High Accretion Rates in Active Galactic Nuclei. XV. Reverberation Mapping of Mg ii Emission Lines[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,2026,282(2).
APA Bai, Hua-Rui.,Du, Pu.,Hu, Chen.,Chen, Yong-Jie.,Yao, Zhu-Heng.,...&Wang, Jian-Min.(2026).Supermassive Black Holes with High Accretion Rates in Active Galactic Nuclei. XV. Reverberation Mapping of Mg ii Emission Lines.ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,282(2).
MLA Bai, Hua-Rui,et al."Supermassive Black Holes with High Accretion Rates in Active Galactic Nuclei. XV. Reverberation Mapping of Mg ii Emission Lines".ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 282.2(2026).

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来源:云南天文台

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