Distribution of the extensive Doppler redshift of quasars
文献类型：期刊论文
| 作者 | Tan YP(覃一平)1,2 ; Liu HT(刘洪涛)1,3; Liang EW(梁恩维)1,2; Dong YM(董云明)1,3; Su CY(苏成悦)1,3,4
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| 刊名 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
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| 出版日期 | 2004-07-11 |
| 卷号 | 351期号:4页码:1319-1326 |
| 关键词 | galaxies : distances and redshifts quasars : absorption lines quasars : emission lines cosmology : observations |
| ISSN号 | 0035-8711 |
| 产权排序 | 第一完成单位 |
| 通讯作者 | Qin, YP (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, POB 110, Kunming 650011, Yunnan, Peoples R China. |
| 英文摘要 | We make an analysis of the distribution of the extensive Doppler redshift defined as (z) over tilde (Dopp) = (z(abs) - z(em)) / (1 + z(em)) with a sample of 1317 absorption redshifts available from 401 quasars. The analysis reveals a bi-peak structure in the distribution, with one component located at (z) over tilde (Dopp) similar or equal to 0.00 and the other at (z) over tilde (Dopp) similar or equal to -0.01. A study of some possible causes suggests that the structure can be well interpreted: while the absorbers inside the same cluster as the quasar concerned could contribute to the first component and the less populated space between clusters could explain the gap between the two peaks, the typical distance between clusters could account for the second component. If the bi-peak structure is real, which needs to be confirmed by complete samples, one would be able to obtain some useful cosmological information. |
| 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] | STELLAR OBJECTS ; ABSORPTION ; CATALOG ; GALAXIES ; SPECTRA ; QSOS |
| 收录类别 | SCI |
| 原文出处 | http://mnras.oxfordjournals.org/content/351/4/1319 |
| 语种 | 英语 |
| WOS记录号 | WOS:000222423400018 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/6973]  |
| 专题 | 云南天文台_星系研究组 |
| 作者单位 | 1.National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, PO Box 110, Kunming, Yunnan, 650011, China 2.Physics Department, Guangxi University, Nanning, Guangxi, 530004, China 3.The Graduate School of the Chinese Academy of Sciences 4.Department of Physics, Guangdong Industrial University, Guangzhou, Guangdong, 510643, China |
| 推荐引用方式 GB/T 7714 | Tan YP,Liu HT,Liang EW,et al. Distribution of the extensive Doppler redshift of quasars[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2004,351(4):1319-1326. |
| APA | Tan YP,Liu HT,Liang EW,Dong YM,&Su CY.(2004).Distribution of the extensive Doppler redshift of quasars.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,351(4),1319-1326. |
| MLA | Tan YP,et al."Distribution of the extensive Doppler redshift of quasars".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 351.4(2004):1319-1326. |
入库方式： OAI收割
来源：云南天文台
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