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SUPERMASSIVE BLACK HOLES WITH HIGH ACCRETION RATES IN ACTIVE GALACTIC NUCLEI. VI. VELOCITY-RESOLVED REVERBERATION MAPPING OF THE H beta LINE
Du, Pu1; Lu, Kai-Xing1,2; Hu, Chen1; Qiu, Jie1; Li, Yan-Rong1; Huang, Ying-Ke1; Wang, Fang3; Bai JM(白金明)3; Bian, Wei-Hao4; Yuan, Ye-Fei5; Ho, Luis C.6,7; Wang, Jian-Min1,8; SEAMBH Collaboration
Source PublicationASTROPHYSICAL JOURNAL
2016-03-20
Volume820Issue:1
DOI10.3847/0004-637X/820/1/27
Contribution Rank第3完成单位
Indexed BySCI
Keywordaccretion, accretion disks galaxies: active quasars: supermassive black holes
Abstract

In the sixth of a series of papers reporting on a large reverberation mapping (RM) campaign of active galactic nuclei (AGNs) with high accretion rates, we present velocity-resolved time lags of H beta emission lines for nine objects observed in the campaign during 2012-2013. In order to correct the line broadening caused by seeing and instruments before analyzing the velocity-resolved RM, we adopt the Richardson-Lucy deconvolution to reconstruct their H beta profiles. The validity and effectiveness of the deconvolution are checked using Monte Carlo simulation. Five among the nine objects show clear dependence of the time delay on velocity. Mrk 335 and Mrk 486 show signatures of gas inflow whereas the clouds in the broad-line regions (BLRs) of Mrk 142 and MCG + 06-26-012 tend to be radial outflowing. Mrk 1044 is consistent with having virialized motions. The lags of the remaining four are not velocity-resolvable. The velocity-resolved RM of super-Eddington accreting massive black holes (SEAMBHs) shows that they have diverse kinematics in their BLRs. Comparing with the AGNs with sub-Eddington accretion rates, we do not find significant differences in the BLR kinematics of SEAMBHs.

Funding ProjectCAS ; People's Government of Yunnan Province ; Strategic Priority Research Program-The Emergence of Cosmological Structures of the Chinese Academy of Sciences[XDB09000000] ; NSFC[NSFC-11173023] ; NSFC[NSFC-11133006] ; NSFC[NSFC-11373024] ; NSFC[NSFC-11233003] ; NSFC[NSFC-11503026] ; NSFC[NSFC-11573026] ; NSFC[NSFC-11473002] ; NSFC-CAS[U1431228] ; China-Israel NSFC-ISF[11361140347] ; Key Research Program of the Chinese Academy of Sciences[KJZD-EW-M06]
Funding OrganizationCAS ; People's Government of Yunnan Province ; Strategic Priority Research Program-The Emergence of Cosmological Structures of the Chinese Academy of Sciences[XDB09000000] ; NSFC[NSFC-11173023, NSFC-11133006, NSFC-11373024, NSFC-11233003, NSFC-11503026, NSFC-11573026, NSFC-11473002] ; NSFC-CAS[U1431228] ; China-Israel NSFC-ISF[11361140347] ; Key Research Program of the Chinese Academy of Sciences[KJZD-EW-M06]
Language英语
Subject Area天文学 ; 天体物理学 ; 高能天体物理学
MOST Discipline Catalogue理学 ; 理学::天文学
SubtypeArticle
PublisherIOP PUBLISHING LTD
Publication PlaceTEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
ISSN0004-637X
URL查看原文
WOS IDWOS:000372787000027
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS KeywordAGN MONITORING PROJECT ; EARLY-TYPE GALAXIES ; SEYFERT 1 GALAXIES ; HIGH-RESOLUTION SPECTROGRAPH ; HUBBLE-SPACE-TELESCOPE ; BROAD EMISSION-LINES ; FE II REVERBERATION ; DATA RELEASE ; DYNAMICAL MODELS ; NEARBY GALAXIES
Citation statistics
Document Type期刊论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/9571
Collection丽江天文观测站(南方基地)
Corresponding AuthorDu, Pu; Wang, Jian-Min
Affiliation1.Key Laboratory for Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, 19B Yuquan Road, Beijing 100049, China
2.Astronomy Department, Beijing Normal University, Beijing 100875, China
3.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China
4.Physics Department, Nanjing Normal University, Nanjing 210097, China
5.Department of Astronomy, University of Science and Technology of China, Hefei 230026, China
6.Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, China
7.Department of Astronomy, School of Physics, Peking University, Beijing 100871, China
8.National Astronomical Observatories of China, Chinese Academy of Sciences, 20A Datun Road, Beijing 100020, China
Recommended Citation
GB/T 7714
Du, Pu,Lu, Kai-Xing,Hu, Chen,et al. SUPERMASSIVE BLACK HOLES WITH HIGH ACCRETION RATES IN ACTIVE GALACTIC NUCLEI. VI. VELOCITY-RESOLVED REVERBERATION MAPPING OF THE H beta LINE[J]. ASTROPHYSICAL JOURNAL,2016,820(1).
APA Du, Pu.,Lu, Kai-Xing.,Hu, Chen.,Qiu, Jie.,Li, Yan-Rong.,...&SEAMBH Collaboration.(2016).SUPERMASSIVE BLACK HOLES WITH HIGH ACCRETION RATES IN ACTIVE GALACTIC NUCLEI. VI. VELOCITY-RESOLVED REVERBERATION MAPPING OF THE H beta LINE.ASTROPHYSICAL JOURNAL,820(1).
MLA Du, Pu,et al."SUPERMASSIVE BLACK HOLES WITH HIGH ACCRETION RATES IN ACTIVE GALACTIC NUCLEI. VI. VELOCITY-RESOLVED REVERBERATION MAPPING OF THE H beta LINE".ASTROPHYSICAL JOURNAL 820.1(2016).
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