The orbital migrations of massive planets in the protoplanetary disks
碩士 === 國立中央大學 === 天文研究所 === 93 === The observed small orbital radii of massive extrasolar planets around the central solar-type stars can be explained by the mechanisms of orbital migration. The scenario is: the planet forms in the protoplanetary disk and induces planet–disk tidal interactions resul...
| Main Authors: | , |
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| Other Authors: | |
| Format: | Others |
| Language: | en_US |
| Published: |
2005
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| Online Access: | http://ndltd.ncl.edu.tw/handle/26707781459636668371 |