A Method for Determining Precisely the Barycentric Position of Uranus Observed with CCD Systems |
| |
Authors: | Peng Qingyu Mao Wei |
| |
Institution: | (1) Yunnan Observatory, Chinese Academy of Sciences, Kunming, 650011, P. R. China |
| |
Abstract: | 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 the Yunnan Observatory.
This revised version was published online in July 2006 with corrections to the Cover Date. |
| |
Keywords: | |
本文献已被 SpringerLink 等数据库收录! |
|