中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
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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