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An ultraluminous quasar with a twelve-billion-solar-mass black hole at redshift 6.30
文献类型：期刊论文
| 作者 | Wu, Xue-Bing1,2; Wang, Feige1,2; Fan, Xiaohui2,3; Yi, Weimin4,5,6; Zuo, Wenwen7 ; Bian, Fuyan8; Jiang, Linhua2; McGreer, Ian D.3; Wang, Ran2; Yang, Jinyi1,2
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| 刊名 | NATURE
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| 出版日期 | 2015-02-26 |
| 卷号 | 518期号:7540页码:512-515 |
| 英文摘要 | So far, roughly 40 quasars with redshifts greater than z = 6 have been discovered(1-8). Each quasar contains a black hole with a mass of about one billion solar masses (10(9) M-circle dot)(2,6,7,9-13). The existence of such black holes when the Universe was less than one billion years old presents substantial challenges to theories of the formation and growth of black holes and the coevolution of black holes and galaxies(14). Here we report the discovery of an ultraluminous quasar, SDSS J010013.02+280225.8, at redshift z = 6.30. It has an optical and near-infrared luminosity a few times greater than those of previously known z > 6 quasars. On the basis of the deep absorption trough(15) on the blue side of the Lyman-alpha emission line in the spectrum, we estimate the proper size of the ionized proximity zone associated with the quasar to be about 26 million light years, larger than found with other z > 6.1 quasars with lower luminosities(16). We estimate (on the basis of a near-infrared spectrum) that the black hole has a mass of similar to 1.2 x 10(10) M-circle dot, which is consistent with the 1.3 x 10(10) M-circle dot derived by assuming an Eddington-limited accretion rate. |
| WOS标题词 | Science & Technology |
| 类目[WOS] | Multidisciplinary Sciences |
| 研究领域[WOS] | Science & Technology - Other Topics |
| 关键词[WOS] | DIGITAL SKY SURVEY ; SIMILAR-TO 6 ; Z-SIMILAR-TO-6 QUASARS ; LUMINOSITY FUNCTION ; SDSS QUASARS ; DATA RELEASE ; MASSES ; EVOLUTION ; DISCOVERY ; EMISSION |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000350097300041 |
| 公开日期 | 2015-08-18 |
| 源URL | [http://119.78.226.72/handle/331011/18209]  |
| 专题 | 上海天文台_星系宇宙学重点实验室 |
| 作者单位 | 1.Peking Univ, Sch Phys, Dept Astron, Beijing 100871, Peoples R China 2.Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China 3.Univ Arizona, Steward Observ, Tucson, AZ 85721 USA 4.Chinese Acad Sci, Yunnan Observ, Kunming 650011, Peoples R China 5.Univ Chinese Acad Sci, Beijing 100049, Peoples R China 6.Chinese Acad Sci, Key Lab Struct & Evolut Celestial Objects, Kunming 650011, Peoples R China 7.Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China 8.Australian Natl Univ, Res Sch Astron & Astrophys, Mt Stromlo Observ, Weston, ACT 2611, Australia 9.Univ Arizona, Large Binocular Telescope Observ, Tucson, AZ 85721 USA 10.Carnegie Inst Sci, Las Campanas Observ, La Serena, Chile |
| 推荐引用方式 GB/T 7714 | Wu, Xue-Bing,Wang, Feige,Fan, Xiaohui,et al. An ultraluminous quasar with a twelve-billion-solar-mass black hole at redshift 6.30[J]. NATURE,2015,518(7540):512-515. |
| APA | Wu, Xue-Bing.,Wang, Feige.,Fan, Xiaohui.,Yi, Weimin.,Zuo, Wenwen.,...&Beletsky, Yuri.(2015).An ultraluminous quasar with a twelve-billion-solar-mass black hole at redshift 6.30.NATURE,518(7540),512-515. |
| MLA | Wu, Xue-Bing,et al."An ultraluminous quasar with a twelve-billion-solar-mass black hole at redshift 6.30".NATURE 518.7540(2015):512-515. |
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