AGN black hole masses and methods to estimate the mass
文献类型:期刊论文
作者 | Xie GZ(谢光中)1,2![]() ![]() ![]() ![]() |
刊名 | PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN
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出版日期 | 2005 |
卷号 | 57期号:1页码:183-186 |
关键词 | active galactic nuclei black hole physics galaxies : fundamental parameters |
ISSN号 | 0004-6264 |
产权排序 | 第一完成单位 |
通讯作者 | Xie, GZ (reprint author), Chinese Acad Sci, Yunnan Observ, Natl Astron Observ, POB 110, Kunming 650011, Peoples R China. |
英文摘要 | The black hole mass, along with the ratio of the accretion rate to the Eddington accretion rate, is a fundamental parameter of active galactic nuclei. Using our new method to estimate the black hole mass, we developed our sample and estimated black hole masses, indicated by M(H) for 12 blazars. We compared 12 cases, for each of which the relevant black hole mass was also estimated by the L(5100)-R(BLR) relation or the M(BH)-sigma correlation method, which is indicated by M(sigma) We also found that (1) M(H) values are systematically lower than M(sigma), but the differences between M(sigma) and M(H) are very small for most sources; (2) there is a significant correlation between M(sigma) and M(H), the correlation coefficient being r = 0.66 with a chance probability of p similar to 1.9 x 10(-2). Based on these properties mentioned above, we have shown that the small systematical difference between M(sigma) and M(H) is probably due to some systematic errors in our method. |
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] | BL-LACERTAE OBJECTS ; ACTIVE GALACTIC NUCLEI ; RAY-LOUD BLAZARS ; SPECTRAL VARIABILITY ; LUMINOSITY ; QUASARS ; GALAXIES ; PHOTOMETRY ; EXOSAT |
收录类别 | SCI |
原文出处 | http://pasj.oxfordjournals.org/content/57/1/183 |
语种 | 英语 |
WOS记录号 | WOS:000229622600015 |
公开日期 | 2016-05-03 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/6998] ![]() |
专题 | 云南天文台_星系研究组 |
作者单位 | 1.National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Science, P.O.Box 110, Kunming 650011, P.R.China 2.Yunnan Astrophysics Center, Yunnan University, Kunming 650091, P.R.China 3.Physics Department, Yunnan Normal University, Kunming 650091, P.R.China 4.Physics Department, Yuxi Normal College, Yuxi 653100, P.R.China 5.The Graduate School of the Chinese Academy of Sciences, Beijing, P.R.China |
推荐引用方式 GB/T 7714 | Xie GZ,Chen LE,Xie, ZH,et al. AGN black hole masses and methods to estimate the mass[J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN,2005,57(1):183-186. |
APA | Xie GZ,Chen LE,Xie, ZH,Ma L,&Zhou SB.(2005).AGN black hole masses and methods to estimate the mass.PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN,57(1),183-186. |
MLA | Xie GZ,et al."AGN black hole masses and methods to estimate the mass".PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN 57.1(2005):183-186. |
入库方式: OAI收割
来源:云南天文台
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