A possible explanation of the gaps in the distribution of the mean motions of the asteroids
Journal
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- Proceedings of the Tokyo Mathematice-Physical Society
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Proceedings of the Tokyo Mathematice-Physical Society 2 264-269, 1918
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Details 詳細情報について
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- CRID
- 1573950398897538176
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- NII Article ID
- 10003841510
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- Data Source
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- CiNii Articles