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REVERBERATION MAPPING OF THE GAMMA-RAY LOUD NARROW-LINE SEYFERT 1 GALAXY 1H 0323+342
Wang F(王放)1,2,3; Du, Pu4; Hu, Chen4; Bai JM(白金明)1,3; Wang CJ(王传军)1,2,3; Yi WM(易卫敏)1,3; Wang JG(王建国)1,3; Zhang JJ(张居甲)1,3; Xin YX(辛玉新)1,3; Lun BL(伦宝利)1,3; Chang L(常亮)1,3; Fan YF(范玉峰)1,3
Source PublicationASTROPHYSICAL JOURNAL
2016-06-20
Volume824Issue:2
DOI10.3847/0004-637X/824/2/149
Contribution Rank第1完成单位
Indexed BySCI
KeywordGalaxies: Active Galaxies: Individual (1h 0323+342) Galaxies: Jets Galaxies: Nuclei
Abstract

Recently, 1H 0323+342 has attracted a lot of attention as one of several narrow-line Seyfert 1 galaxies detected in the gamma-ray band. To understand their central energy engines and jet phenomena, the black hole mass is important. We made use of the Lijiang 2.4 m Telescope to monitor 1H 0323+342 for more than two months. This galaxy is one of the candidates for a monitoring project of super-Eddington accreting massive black holes. The reverberation mapping shows that H beta emission has a delayed response of 14.8(-2.7)(+3.9) days with respect to the SDSS g' light curve in the rest frame. The optical Fe II variations were detected after subtracting host contaminations, and a reverberation with a delay of 15.2(-4.1)(+7.4) days was found in the rest frame. By assuming the viral factor f(BLR) = 6.17 for the broadline region (BLR) velocity characterized by FWHM because of the face-on orientation, we find that the black hole mass derived from H beta is M-center dot = 3.4(-0.6)(+0.9) x 10(7)M(circle dot), and the accretion rate is (M) over dot = 1.11(-0.47)(+0.69), where (M) over dot = (M) over dot(center dot)c(2)/L-Edd, (M) over dot(center dot) is the mass accretion rate, L-Edd is the Eddington luminosity, and c is the speed of light. This black hole is one order less massive than that given by the Magorrian relation from the bulge mass. We test the relation between accretion rates and radio-loudnesses in all mapped radio-loud active galactic nuclei, and find that 1H 0323+342 falls within this group.

Funding ProjectNational Science Foundation of China (NSFC)[11303085] ; National Science Foundation of China (NSFC)[11403096] ; National Science Foundation of China (NSFC)[11573067] ; Strategic Priority Research Program "The Emergence of Cosmological Structures" of the CAS[XDB09000000] ; Key Research Program of the CAS[KJZD-EW-M06] ; CAS "Light of West China" Program ; CAS ; People's Government of Yunnan Province
Funding OrganizationNational Science Foundation of China (NSFC)[11303085, 11403096, 11573067] ; Strategic Priority Research Program "The Emergence of Cosmological Structures" of the CAS[XDB09000000] ; Key Research Program of the CAS[KJZD-EW-M06] ; CAS "Light of West China" Program ; CAS ; People's Government of Yunnan Province
Language英语
Subject Area天文学 ; 星系与宇宙学
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
Archive Date2016-12-15
WOS IDWOS:000381912800085
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS KeywordActive Galactic Nuclei ; Supermassive Black-holes ; High Accretion Rates ; Agn Monitoring Project ; Bl Lacertae Objects ; Space-telescope Survey ; Host Galaxies ; Radio-loud ; Electromagnetic Extraction ; Observational Evidence
Citation statistics
Document Type期刊论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/9687
Collection丽江天文观测站(南方基地)
中国科学院天体结构与演化重点实验室
Corresponding AuthorWang F(王放)
Affiliation1.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, Yunnan, China
2.University of Chinese Academy of Sciences, Beijing 100049, China
3.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650011, Yunnan, China
4.Key Laboratory for Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, 19B Yuquan Road, Beijing 100049, China
First Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Corresponding Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Wang F,Du, Pu,Hu, Chen,et al. REVERBERATION MAPPING OF THE GAMMA-RAY LOUD NARROW-LINE SEYFERT 1 GALAXY 1H 0323+342[J]. ASTROPHYSICAL JOURNAL,2016,824(2).
APA Wang F.,Du, Pu.,Hu, Chen.,Bai JM.,Wang CJ.,...&Fan YF.(2016).REVERBERATION MAPPING OF THE GAMMA-RAY LOUD NARROW-LINE SEYFERT 1 GALAXY 1H 0323+342.ASTROPHYSICAL JOURNAL,824(2).
MLA Wang F,et al."REVERBERATION MAPPING OF THE GAMMA-RAY LOUD NARROW-LINE SEYFERT 1 GALAXY 1H 0323+342".ASTROPHYSICAL JOURNAL 824.2(2016).
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