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. VI. VELOCITY-RESOLVED REVERBERATION MAPPING OF THE H beta LINE

文献类型:期刊论文

作者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
刊名ASTROPHYSICAL JOURNAL
出版日期2016-03-20
卷号820期号:1
关键词accretion, accretion disks galaxies: active quasars: supermassive black holes
ISSN号0004-637X
产权排序第三完成单位
通讯作者Du, P
英文摘要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.
WOS标题词Science & Technology ; Physical Sciences
学科主题Astronomy & Astrophysics
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]AGN 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
收录类别SCI
原文出处http://iopscience.iop.org/article/10.3847/0004-637X/820/1/27/meta
语种英语
WOS记录号WOS:000372787000027
源URL[http://ir.ynao.ac.cn/handle/114a53/9571]  
专题云南天文台_丽江天文观测站(南方基地)
作者单位1.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
推荐引用方式
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).

入库方式: OAI收割

来源:云南天文台

浏览0
下载0
收藏0
其他版本

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。