Cosmic star formation history associated with quasar activity: An approach using the black hole-to-bulge mass correlation
文献类型：期刊论文
| 作者 | Wang, YP; Yamada, T; Taniguchi, Y |
| 刊名 | ASTROPHYSICAL JOURNAL
 |
| 出版日期 | 2003-05-01 |
| 卷号 | 588期号:1页码:113-118 |
| 关键词 | dust, extinction galaxies : active galaxies : elliptical and lenticular, cD galaxies : evolution quasars : general |
| 英文摘要 | The tight correlation between the masses of central black holes and their host spheroids in nearby galaxies and active galactic nuclei (AGNs) suggests that black hole growth is closely related to their spheroid formation. Based on our previous work regarding such a joint evolutionary scheme and the consequential black hole-to-bulge mass correlation, we use the X-ray luminosity function of AGN and the cosmological evolution rate, which are from ROSAT X-ray surveys, to estimate the cosmic star formation history associated with the black hole growth. By the basic assumption that the major black hole growth occurs during the luminous AGN phase, the luminosity function of AGNs as a function of redshift traces not only the accretion history of the black holes but also the cosmic star formation history of the spheroids. Although the space density of the especially luminous quasars is very low, we show that the total amount of star formation associated with the massive black hole growth is almost the same as that of Lyman break galaxies detected by the current optical deep surveys. We thus argue that the optical deep surveys may miss about half of the net star formation in our universe. This is probably due in part to significant dust extinction, as well as the small field of view of previous optical surveys, which cannot sample such rare events with relatively short timescale. However, the far-infrared emission from the dust heated by ongoing star formation during the black hole growth could sufficiently account for the observed SCUBA number counts and would be the probable dominating energy source of the SCUBA population. |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | HUBBLE DEEP FIELD ; ULTRALUMINOUS INFRARED GALAXIES ; LYMAN-BREAK GALAXIES ; X-RAY ; SPIRAL GALAXIES ; GALACTIC NUCLEI ; HIGH-REDSHIFT ; LUMINOSITY FUNCTION ; ENERGY-DISTRIBUTIONS ; MOLECULAR GAS |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000182451800009 |
| 源URL | [http://libir.pmo.ac.cn/handle/332002/15814]  |
| 专题 | 紫金山天文台_暗物质和空间天文实验室 |
| 作者单位 | 1.Acad Sinica, Purple Mt Observ, Nanjing 210008, Peoples R China 2.Natl Astron Observ China, Beijing, Peoples R China 3.Natl Astron Observ Japan, Mitaka, Tokyo, Japan 4.Tohoku Univ, Aoba Ku, Sendai, Miyagi 9808578, Japan |
| 推荐引用方式 GB/T 7714 | Wang, YP,Yamada, T,Taniguchi, Y. Cosmic star formation history associated with quasar activity: An approach using the black hole-to-bulge mass correlation[J]. ASTROPHYSICAL JOURNAL,2003,588(1):113-118. |
| APA | Wang, YP,Yamada, T,&Taniguchi, Y.(2003).Cosmic star formation history associated with quasar activity: An approach using the black hole-to-bulge mass correlation.ASTROPHYSICAL JOURNAL,588(1),113-118. |
| MLA | Wang, YP,et al."Cosmic star formation history associated with quasar activity: An approach using the black hole-to-bulge mass correlation".ASTROPHYSICAL JOURNAL 588.1(2003):113-118. |
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来源：紫金山天文台
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