A method for determining precisely the barycentric position of Uranus observed with CCD systems
文献类型：期刊论文
| 作者 | Peng QY(彭青玉) ; Mao Y(冒蔚)
|
| 刊名 | ASTROPHYSICS AND SPACE SCIENCE
 |
| 出版日期 | 1998 |
| 卷号 | 257期号:2页码:279-285 |
| ISSN号 | 0004-640X |
| 产权排序 | 第一完成单位 |
| 通讯作者 | Peng, QY |
| 英文摘要 | A method for determining precisely the barycentric position of Uranus by CCD systems is presented in this present article. It is required according to the method that the CCD observations obtained both with a long-focus telescope which is used to observe the major satellites of Uranus and with a meridian circle which works in a CCD drift scanning manner when it is used to observe some faint stars. The key part of the method is tested by the observations obtained with the 1-meter telescope at tilt Yunnan Observatory. |
| 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] | EXTRAGALACTIC REFERENCE FRAME ; URANIAN SATELLITES ; PLANETS |
| 收录类别 | SCI |
| 原文出处 | http://link.springer.com/article/10.1023%2FA%3A1001198113600 |
| 语种 | 英语 |
| WOS记录号 | WOS:000078395200010 |
| 公开日期 | 2016-05-03 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/6635]  |
| 专题 | 云南天文台_天体测量及应用研究组 |
| 作者单位 | Yunnan Observatory, Chinese Academy of Sciences, Kunming, 650011, P. R. China |
| 推荐引用方式 GB/T 7714 | Peng QY,Mao Y. A method for determining precisely the barycentric position of Uranus observed with CCD systems[J]. ASTROPHYSICS AND SPACE SCIENCE,1998,257(2):279-285. |
| APA | Peng QY,&Mao Y.(1998).A method for determining precisely the barycentric position of Uranus observed with CCD systems.ASTROPHYSICS AND SPACE SCIENCE,257(2),279-285. |
| MLA | Peng QY,et al."A method for determining precisely the barycentric position of Uranus observed with CCD systems".ASTROPHYSICS AND SPACE SCIENCE 257.2(1998):279-285. |
入库方式： OAI收割
来源：云南天文台
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