Supermassive Black Holes with High Accretion Rates in Active Galactic Nuclei. VII. Reconstruction of Velocity-delay Maps by the Maximum Entropy Method

被引：21

作者：

Xiao, Ming ^{[1
,2
,3
]}

Du, Pu ^{[2
]}

Horne, Keith ^{[4
]}

Hu, Chen ^{[2
]}

Li, Yan-Rong ^{[2
]}

Huang, Ying-Ke ^{[2
]}

Lu, Kai-Xing ^{[1
]}

Qiu, Jie ^{[2
]}

Wang, Fang ^{[1
]}

Bai, Jin-Ming ^{[1
]}

Bian, Wei-Hao ^{[5
]}

Ho, Luis C. ^{[6
,7
]}

Yuan, Ye-Fei ^{[8
]}

Wang, Jian-Min ^{[2
,3
,9
]}

机构：

[1] Chinese Acad Sci, Yunnan Observ, Kunming 650011, Yunnan, Peoples R China

[2] Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, 19B Yuquan Rd, Beijing 100049, Peoples R China

[3] Univ Chinese Acad Sci, 19A Yuquan Rd, Beijing 100049, Peoples R China

[4] Univ St Andrews, SUPA Phys & Astron, St Andrews KY16 9SS, Fife, Scotland

[5] Nanjing Normal Univ, Phys Dept, Nanjing 210097, Jiangsu, Peoples R China

[6] Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China

[7] Peking Univ, Sch Phys, Dept Astron, Beijing 100871, Peoples R China

[8] Univ Sci & Technol China, Dept Astron, Hefei 230026, Anhui, Peoples R China

[9] Chinese Acad Sci, Natl Astron Observ China, 20A Datun Rd, Beijing 100020, Peoples R China

来源：

ASTROPHYSICAL JOURNAL | 2018年 / 864卷 / 02期

基金：

美国国家科学基金会; 国家重点研发计划;

关键词：

accretion; accretion disks; galaxies: active; galaxies: nuclei; galaxies: Seyfert; AGN MONITORING PROJECT; BROAD-LINE REGION; REVERBERATION MAPPING DATA; SEYFERT-GALAXIES; MASS; VARIABILITY; QUASARS;

D O I：

10.3847/1538-4357/aad5e1

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

As one of a series of papers reporting on a large reverberation mapping campaign, we apply the maximum entropy method (MEM) to nine narrow- line Seyfert 1 galaxies with super-Eddington accretion rates observed during 2012-2013 for the velocity-delay maps of their H beta and H gamma emission lines. The maps of six objects are reliably reconstructed using MEM. The maps of H beta and H gamma emission lines of Mrk 335 indicate that the gas of its broad-line region (BLR) is infalling. For Mrk 142, its H beta and H gamma lines show signatures of outflow. The H beta and H gamma maps of Mrk 1044 demonstrate complex kinematics-a virialized motion accompanied by an outflow signature, and the H beta map of IRAS F12397+3333 is consistent with a disk or a spherical shell. The H beta maps of Mrk 486 and MCG +06-26-012 suggest the presence of inflow and outflow, respectively. These super-Eddington accretors show diverse geometry and kinematics. Brief discussions of their BLRs are provided for each individual object.

引用

页数：13

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