| Broad-line Region of the Quasar PG 2130+099 from a Two-year Reverberation Mapping Campaign with High Cadence | |
Hu, Chen1; Li, Yan-Rong1; Du, Pu1; Zhang, Zhi-Xiang1,3; Li, Sha-Sha1,3; Huang, Ying-Ke1,3; Lu KX(卢开兴)4 ; Bai JM(白金名)4; Ho, Luis C.5,6; Bian, Wei-Hao7; Brotherton, Michael S.8; Yuan,Ye-Fei3; Aceituno, Jesús9,10; Winkler, Hartmut11; Wang, Jian-Min1,2,12
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| 通讯作者 | Hu, Chen([email protected]) |
| 发表期刊 | ASTROPHYSICAL JOURNAL
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| 2020-02-10 | |
| 卷号 | 890期号:1页码:13 |
| DOI | 10.3847/1538-4357/ab6a17 |
| 产权排序 | 第4完成单位 |
| 收录类别 | SCI |
| 摘要 | As one of the most interesting Seyfert 1 galaxies, PG 2130+099 has been the target of several reverberation mapping (RM) campaigns over the years. However, its measured broad H beta line responses have been inconsistent, with time lags of similar to 200 days, similar to 25 days, and similar to 10 days being reported for different epochs while its optical luminosity changed no more than 40%. To investigate this issue, we conducted a new RM-campaign with homogenous and high cadence (about similar to 3 days) for two years during 2017-2019 to measure the kinematics and structure of the ionized gas. We successfully detected time lags of broad H beta, He II, He I, and Fe II lines with respect to the varying 5100 angstrom continuum, revealing a stratified structure that is likely virialized with Keplerian kinematics in the first year of observations, but an inflow kinematics of the broad-line region from the second year. With a central black hole mass of 0.97(-0.18)(+0.15) x 10(7)M(circle dot), PG 2130+099 has an accretion rate of 10(2.1 +/- 0.5)L(Edd)c(-2), where L-Edd is the Eddington luminosity and c is speed of light, implying that it is a super-Eddington accretor and likely possesses a slim, rather than thin, accretion disk. The fast changes of the ionization structures of the three broad lines remain puzzling. |
| 资助项目 | Chinese Academy of Sciences (CAS) ; People's Government of Yunnan Province ; Ministry of Science and Technology of China[2016YFA0400700] ; NSFC[NSFC-11773029] ; NSFC[NSFC-11833008] ; NSFC[NSFC-11991054] ; NSFC[NSFC-11922304] ; NSFC[NSFC-11873048] ; NSFC[NSFC-11690024] ; NSFC[NSFC-11703077] ; CAS Key Research Program[KJZD-EW-M06] ; Key Research Program of Frontier Sciences, CAS[QYZDJ-SSWSLH007] |
| 项目资助者 | Chinese Academy of Sciences (CAS) ; People's Government of Yunnan Province ; Ministry of Science and Technology of China[2016YFA0400700] ; NSFC[NSFC-11773029, NSFC-11833008, NSFC-11991054, NSFC-11922304, NSFC-11873048, NSFC-11690024, NSFC-11703077] ; CAS Key Research Program[KJZD-EW-M06] ; Key Research Program of Frontier Sciences, CAS[QYZDJ-SSWSLH007] |
| 语种 | 英语 |
| 学科领域 | 天文学 ; 天体物理学 ; 高能天体物理学 |
| 文章类型 | Article |
| 出版者 | IOP PUBLISHING LTD |
| 出版地 | TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND |
| ISSN | 0004-637X |
| URL | 查看原文 |
| WOS记录号 | WOS:000522096700003 |
| WOS研究方向 | Astronomy & Astrophysics |
| WOS类目 | Astronomy & Astrophysics |
| 关键词[WOS] | ACTIVE GALACTIC NUCLEI ; SUPERMASSIVE BLACK-HOLES ; SEYFERT-GALAXIES ; EMISSION ; VARIABILITY ; MASS ; CONTINUUM ; SIZE ; GAS |
| 引用统计 | |
| 文献类型 | 期刊论文 |
| 条目标识符 | http://ir.ynao.ac.cn/handle/114a53/22302 |
| 专题 | 南方基地 |
| 通讯作者 | Hu, Chen |
| 作者单位 | 1.Key Laboratory for Particle Astrophysics, Institute of High Energy Physics, The Chinese Academy of Sciences, 19B Yuquan Road, Beijing 100049, People's Republic of China 2.School of Astronomy and Space Science, University of Chinese Academy of Sciences, 19A Yuquan Road, Beijing 100049, People’s Republic of China 3.Department of Astronomy, University of Science and Technology of China, Hefei 230026, People’s Republic of China 4.Yunnan Observatories, The Chinese Academy of Sciences, Kunming 650011, People’s Republic of China 5.Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, People’s Republic of China 6.Department of Astronomy, School of Physics, Peking University, Beijing 100871, People’s Republic of China 7.Physics Department, Nanjing Normal University, Nanjing 210097, People’s Republic of China 8.Department of Physics and Astronomy, University of Wyoming, Laramie, WY 82071, USA 9.Centro Astronomico Hispano Alemán, Sierra de los filabres sn, E-04550 Gergal, Almería, Spain 10.Instituto de Astrofísica de Andalucía, Glorieta de la astronomía sn, E-18008 Granada, Spain 11.Department of Physics, University of Johannesburg, P.O. Box 524, 2006 Auckland Park, South Africa 12.National Astronomical Observatories of China, The Chinese Academy of Sciences, 20A Datun Road, Beijing 100020, People’s Republic of China |
| 推荐引用方式 GB/T 7714 | Hu, Chen,Li, Yan-Rong,Du, Pu,et al. Broad-line Region of the Quasar PG 2130+099 from a Two-year Reverberation Mapping Campaign with High Cadence[J]. ASTROPHYSICAL JOURNAL,2020,890(1):13. |
| APA | Hu, Chen.,Li, Yan-Rong.,Du, Pu.,Zhang, Zhi-Xiang.,Li, Sha-Sha.,...&Wang, Jian-Min.(2020).Broad-line Region of the Quasar PG 2130+099 from a Two-year Reverberation Mapping Campaign with High Cadence.ASTROPHYSICAL JOURNAL,890(1),13. |
| MLA | Hu, Chen,et al."Broad-line Region of the Quasar PG 2130+099 from a Two-year Reverberation Mapping Campaign with High Cadence".ASTROPHYSICAL JOURNAL 890.1(2020):13. |
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| Broad-line Region of（1616KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 | |
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