A possible mechanism for the mass ratio limitation in early type galaxies
文献类型:期刊论文
作者 | Wang, YP; Biermann, PL |
刊名 | ASTRONOMY & ASTROPHYSICS
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出版日期 | 1998-06-01 |
卷号 | 334期号:1页码:87-95 |
关键词 | galaxies : nuclei galaxies : evolution galaxies : formation galaxies : starburst galaxies : elliptical and lenticular, cD |
ISSN号 | 0004-6361 |
英文摘要 | There is an interesting correlation between the central objects and their host galaxies in recent high resolution HST photometry of early type galaxies and Near-IR images of nearby quasar hosts. It has been shown that a) the hosts of these very luminous quasars are likely to be early type galaxies and that b) the mass ratio of central black holes (BHs) and their host spheroidal components (M-bh/M-spheroid) is similar to 0.002 within a factor of three. Using the hierarchical galaxy evolution scheme for the formation of early-type galaxies, we present here a general viscous accretion disk model to trace the star formation and central engine evolution before and after mergers. In our model, starbursts and AGN coexist; these two activities compete for the gas supply, interact with each other, probably feed back on each other and lock into a final status. They thus constrain the ratio of central black hole mass and its host spheroidal mass to a universal value of order 10(-3). |
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] | ACTIVE GALACTIC NUCLEI ; QUASAR HOST GALAXIES ; SPIRAL GALAXIES ; STAR-FORMATION ; DISK GALAXIES ; BLACK-HOLES ; ELLIPTICAL GALAXIES ; CHEMICAL EVOLUTION ; MERGING GALAXIES ; MERGER MODEL |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000074072100017 |
公开日期 | 2013-02-05 |
源URL | [http://libir.pmo.ac.cn/handle/332002/8369] ![]() |
专题 | 紫金山天文台_期刊(老文献) |
作者单位 | 1.Max Planck Inst Radioastron, D-53121 Bonn, Germany 2.Acad Sinica, Purple Mt Observ, Nanjing 210008, Peoples R China |
推荐引用方式 GB/T 7714 | Wang, YP,Biermann, PL. A possible mechanism for the mass ratio limitation in early type galaxies[J]. ASTRONOMY & ASTROPHYSICS,1998,334(1):87-95. |
APA | Wang, YP,&Biermann, PL.(1998).A possible mechanism for the mass ratio limitation in early type galaxies.ASTRONOMY & ASTROPHYSICS,334(1),87-95. |
MLA | Wang, YP,et al."A possible mechanism for the mass ratio limitation in early type galaxies".ASTRONOMY & ASTROPHYSICS 334.1(1998):87-95. |
入库方式: OAI收割
来源:紫金山天文台
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