碩士 / 國立中央大學 / 物理與天文研究所 / 99 / The origin of the high inclination and large eccentricity population of the Trans-Neptunian Objects (TNOs) has been interpreted in terms of the gravitational scattering e ect of a
large planet, several large planetoids, or passing stars (Gomes, 2009). For the passing star scenario which would be most aptly applied to the case if the sun formed in a star cluster, We have developed models to simulate situations of gravitational interaction of proto-planetary systems surrounding low-mass stars in a dense stellar environment. We found passing stars with perihelion distaces on the order of a few hundred AU could excite
TNOs to high inclination orbits.
| Identifer | oai:union.ndltd.org:TW/099NCU05197001 |
| Date | January 2010 |
| Creators | Yongsin Tsao, 曹永新 |
| Contributors | Wing-Huen Ip, 葉永烜 |
| Source Sets | National Digital Library of Theses and Dissertations in Taiwan |
| Language | zh-TW |
| Detected Language | English |
| Type | 學位論文 ; thesis |
| Format | 42 |
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