Broad-line Region of the Quasar PG 2130+099 from a Two-year Reverberation Mapping Campaign with High Cadence

doi:10.3847/1538-4357/ab6a17

CORC > 云南天文台 > 中国科学院云南天文台 > 丽江天文观测站（南方基地）

	Broad-line Region of the Quasar PG 2130+099 from a Two-year Reverberation Mapping Campaign with High Cadence
	Hu, Chen 1; Li, Yan-Rong 1; Du, Pu 1; Zhang, Zhi-Xiang 1,12; Li, Sha-Sha 1,12; Huang, Ying-Ke 1,12; Lu KX(卢开兴)11; Bai JM(白金名)11; Ho, Luis C.5,6; Bian, Wei-Hao 8
刊名	ASTROPHYSICAL JOURNAL
	2020-02-10
卷号	890 期号:1 页码:13
ISSN号	0004-637X
DOI	10.3847/1538-4357/ab6a17
通讯作者	Hu, Chen(huc@ihep.ac.cn)
产权排序	第4完成单位
文献子类	Article
英文摘要	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.
学科主题	天文学 ; 天体物理学 ; 高能天体物理学
URL标识	查看原文
出版地	TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
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]
WOS关键词	ACTIVE GALACTIC NUCLEI ; SUPERMASSIVE BLACK-HOLES ; SEYFERT-GALAXIES ; EMISSION ; VARIABILITY ; MASS ; CONTINUUM ; SIZE ; GAS
WOS研究方向	Astronomy & Astrophysics
语种	英语
出版者	IOP PUBLISHING LTD
WOS记录号	WOS:000522096700003
资助机构	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]
内容类型	期刊论文
源URL	[http://ir.ynao.ac.cn/handle/114a53/22301]
专题	云南天文台_丽江天文观测站（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.Centro Astronomico Hispano Alemán, Sierra de los filabres sn, E-04550 Gergal, Almería, Spain 4.Department of Physics, University of Johannesburg, P.O. Box 524, 2006 Auckland Park, South Africa 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.Department of Physics and Astronomy, University of Wyoming, Laramie, WY 82071, USA 8.Physics Department, Nanjing Normal University, Nanjing 210097, People’s Republic of China 9.National Astronomical Observatories of China, The Chinese Academy of Sciences, 20A Datun Road, Beijing 100020, People’s Republic of China 10.Instituto de Astrofísica de Andalucía, Glorieta de la astronomía sn, E-18008 Granada, Spain
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.