Black hole to bulge mass correlation in Active Galactic Nuclei: a test for the simple unified formation scheme
文献类型：期刊论文
| 作者 | Wang, YP; Biermann, PL; Wandel, A |
| 刊名 | ASTRONOMY & ASTROPHYSICS
 |
| 出版日期 | 2000-09-01 |
| 卷号 | 361期号:2页码:550-554 |
| 关键词 | galaxies : interactions galaxies : Seyfert galaxies : quasars : general galaxies : elliptical and lenticular, cD galaxies : formation |
| ISSN号 | 0004-6361 |
| 英文摘要 | A mass correlation of central black holes and their spheroids similar to 0.002 (within a factor of three) is suggested by Hubble Space Telescope (HST) and various ground-based CCD photometries of early type galaxies. The near-IR images of quasar hosts and the emission line measurements of Broad Line Region for bright QSOs present a similar correlation, which supports the speculation of an evolutionary linkage between the early active QSO phase and the central black holes in normal galaxies. On the other hand, recent reverberation mapping of a sample of Seyferts shows a broad distribution of black hole to bulge mass ratio with a mean of similar to 10(-3.5), about one magnitude lower than the value in early type galaxies and bright QSOs. Adopting a simple unified formation scheme for QSOs and Seyferts, we will discuss in this letter the dependence of the black hole to bulge mass ratio in Active Galactic Nuclei (AGNs) on the environmental parameters of the host galaxies. We show a broad distribution of the mass correlation could be due to different velocity dispersion of the accreting gas from different Formation mechanism, and the mass ratio in normal galaxies and bright QSOs is probably a limit case of black hole evolution by merger enhanced accretion close to Eddington limit. |
| 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] | ULTRALUMINOUS INFRARED GALAXIES ; SEYFERT-GALAXIES ; QUASARS ; MERGERS ; MECHANISM ; CENTERS ; NGC4258 ; ORIGIN ; DISKS |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000089926000018 |
| 公开日期 | 2013-02-01 |
| 源URL | [http://libir.pmo.ac.cn/handle/332002/8290]  |
| 专题 | 紫金山天文台_期刊（老文献） |
| 作者单位 | 1.Acad Sinica, Purple Mt Observ, Nanjing 210008, Peoples R China 2.Chinese Acad Sci, Natl Astron Observ, Beijing 100864, Peoples R China 3.Max Planck Inst Radioastron, D-53121 Bonn, Germany 4.Hebrew Univ Jerusalem, Racah Inst Phys, IL-91904 Jerusalem, Israel |
| 推荐引用方式 GB/T 7714 | Wang, YP,Biermann, PL,Wandel, A. Black hole to bulge mass correlation in Active Galactic Nuclei: a test for the simple unified formation scheme[J]. ASTRONOMY & ASTROPHYSICS,2000,361(2):550-554. |
| APA | Wang, YP,Biermann, PL,&Wandel, A.(2000).Black hole to bulge mass correlation in Active Galactic Nuclei: a test for the simple unified formation scheme.ASTRONOMY & ASTROPHYSICS,361(2),550-554. |
| MLA | Wang, YP,et al."Black hole to bulge mass correlation in Active Galactic Nuclei: a test for the simple unified formation scheme".ASTRONOMY & ASTROPHYSICS 361.2(2000):550-554. |
入库方式： OAI收割
来源：紫金山天文台
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