Dependence of the broad Fe K alpha line on the physical parameters of AGN | |
Liu, Zhu1,2; Yuan, Weimin1,2; Lu, Youjun2,3; Carrera, Francisco J.4; Falocco, Serena6; Dong XB(董小波)6,7 | |
刊名 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY |
2016-11-21 | |
卷号 | 463期号:1页码:684-695 |
关键词 | galaxies: active X-rays: galaxies |
ISSN号 | 0035-8711 |
通讯作者 | Liu, Z ; Yuan, WM |
产权排序 | 第六完成单位 |
英文摘要 | In this paper, the dependence of the broad Fe K alpha line on the physical parameters of AGN, such as the black hole mass M-BH, accretion rate (equivalently represented by Eddington ratio lambda(Edd)) and optical classification is investigated by applying the X-ray spectra stacking method to a large sample of AGN which have well measured optical parameters. A broad-line feature is detected (> 3 sigma) in the stacked spectra of the high lambda(Edd) sub-sample (log lambda(Edd) > -0.9). The profile of the broad line can be well fitted with relativistic broad-line model, with the line energy consistent with highly ionized Fe K alpha line (i.e. Fe xxvi). A model consisting of multiple narrow lines cannot be ruled out, however. We found hints that the Fe K line becomes broader as the lambda(Edd) increases. No broad-line feature is shown in the sub-sample of broad-line Seyfert 1 (BLS1) galaxies and in the full sample, while a broad line might be present, though at low significance, in the sub-sample of narrow-line Seyfert 1 (NLS1) galaxies. We find no strong dependence of the broad line on black hole masses. Our results indicate that the detection/properties of the broad Fe K alpha line may strongly depend on lambda(Edd), which can be explained if the ionization state and/or truncation radius of the accretion disc changes with lambda(Edd). The non-detection of the broad line in the BLS1 sub-sample can be explained if the average equivalent width of the relativistic Fe K alpha line is weak or/and the fraction of sources with relativistic Fe K alpha line is small in BLS1 galaxies. |
学科主题 | Astronomy & Astrophysics |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | ACTIVE GALACTIC NUCLEI ; ADVECTION-DOMINATED ACCRETION ; DIGITAL SKY SURVEY ; SEYFERT 1 GALAXIES ; PHOTON IMAGING CAMERA ; 2XMM CATALOG SOURCES ; MASSIVE BLACK-HOLE ; RAY SPECTRAL SLOPE ; XMM-NEWTON ; EDDINGTON RATIO |
收录类别 | SCI |
原文出处 | http://mnras.oxfordjournals.org/content/463/1/684 |
语种 | 英语 |
WOS记录号 | WOS:000386464900055 |
内容类型 | 期刊论文 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/9754] |
专题 | 云南天文台_丽江天文观测站(南方基地) 云南天文台_中国科学院天体结构与演化重点实验室 |
作者单位 | 1.Key Laboratory of Space Astronomy and Technology, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China 2.University of Chinese Academy of Sciences, School of Astronomy and Space Science, Beijing 100049, China 3.National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China 4.Instituto de Física de Cantabria (CSIC-UC), Avenida de los Castros, E-39005 Santander, Spain 5.KTH Royal Institute of Technology, Department of Physics and the Oskar Klein Centre, AlbaNova, SE-106 91 Stockholm, Sweden 6.Yunnan Observatories, Chinese Academy of Sciences, Kunming, Yunnan 650011, China 7.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming, Yunnan 650011, China |
推荐引用方式 GB/T 7714 | Liu, Zhu,Yuan, Weimin,Lu, Youjun,et al. Dependence of the broad Fe K alpha line on the physical parameters of AGN[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2016,463(1):684-695. |
APA | Liu, Zhu,Yuan, Weimin,Lu, Youjun,Carrera, Francisco J.,Falocco, Serena,&Dong XB.(2016).Dependence of the broad Fe K alpha line on the physical parameters of AGN.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,463(1),684-695. |
MLA | Liu, Zhu,et al."Dependence of the broad Fe K alpha line on the physical parameters of AGN".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 463.1(2016):684-695. |
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