The Existence and Orbital Stability of Planets in 16 Cygni B System
碩士 === 國立清華大學 === 天文研究所 === 97 === The radial velocity measurement is a popular method to detect exoplanets in recent year. About 95% of discovered exoplanets were found by this method. According to the periodic velocity variation of the host star, we can predict the possible mass, eccentricity, and...
| Main Authors: | , |
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| Format: | Others |
| Language: | en_US |
| Published: |
2009
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| Online Access: | http://ndltd.ncl.edu.tw/handle/48840506819116687951 |