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
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| 出版日期 | 2026-02-01 |
| 卷号 | 282期号:2 |
| ISSN号 | 0067-0049 |
| DOI | 10.3847/1538-4365/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; |
| 推荐引用方式 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). |
入库方式: OAI收割
来源:云南天文台
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