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A method for determining precisely the barycentric position of Uranus observed with CCD systems
Peng QY(彭青玉); Mao Y(冒蔚); Peng, QY
发表期刊ASTROPHYSICS AND SPACE SCIENCE
1998
卷号257期号:2页码:279-285
DOI10.1023/A:1001198113600
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收录类别SCI
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.
语种英语
学科领域Astronomy & Astrophysics
文章类型Article
ISSN0004-640X
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WOS记录号WOS:000078395200010
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]EXTRAGALACTIC REFERENCE FRAME ; URANIAN SATELLITES ; PLANETS
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文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/6635
专题天体测量及应用研究组
通讯作者Peng, QY
作者单位Yunnan Observatory, Chinese Academy of Sciences, Kunming, 650011, P. R. China
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Peng QY,Mao Y,Peng, QY. 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,&Peng, QY.(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.
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