The Difference between the α-disks of Seyfert 1 Galaxiesand Quasars
文献类型:期刊论文
作者 | Bian Weihao2; Hong Dong1; Zhao Yongheng2 |
刊名 | 中国天文和天体物理学报:英文版 |
出版日期 | 2004 |
卷号 | 4.0期号:1.0页码:61 |
ISSN号 | 1009-9271 |
关键词 | 黑洞 磁倾角 类星体 星系 核子 光学 发光度 赛弗特星系 |
英文摘要 | In a previous paper, it was suggested that contamination of the nuclear lumiuosity by the host galaxy plays an important role in determining the parameters of the standard a disk of AGNs. Using the nuclear absolute B band magnitud einstead of the total absolute B band magnitude, we have recalculated the central black hole masses, accretion rates and disk inclinations for 20 Seyfert 1 galaxies and 17 Palomar-Green (PG) quasars. It is found that a small value of a is needed for the Seyfert 1 galaxies than for the PG quasars. This difference in a possibly leads to the different properties of Seyfert 1 galaxies and quasars. Furthermore, we find most of the objects in this sample are not accreting at super-Eddington rates if we adopt the nuclear optical luminosity in our calculation. |
语种 | 英语 |
源URL | [http://ir.bao.ac.cn/handle/114a11/60347] |
专题 | 光学部_LAMOST运行和发展中心 |
作者单位 | 1.哥伦比亚大学教育学院 2.中国科学院国家天文台 |
推荐引用方式 GB/T 7714 | Bian Weihao,Hong Dong,Zhao Yongheng. The Difference between the α-disks of Seyfert 1 Galaxiesand Quasars[J]. 中国天文和天体物理学报:英文版,2004,4.0(1.0):61. |
APA | Bian Weihao,Hong Dong,&Zhao Yongheng.(2004).The Difference between the α-disks of Seyfert 1 Galaxiesand Quasars.中国天文和天体物理学报:英文版,4.0(1.0),61. |
MLA | Bian Weihao,et al."The Difference between the α-disks of Seyfert 1 Galaxiesand Quasars".中国天文和天体物理学报:英文版 4.0.1.0(2004):61. |
入库方式: OAI收割
来源:国家天文台
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