Simulation of the Stochastic Star FormationHistories in Galactic Bulge and Disk
碩士 === 國立中央大學 === 天文研究所 === 90 === Recent observations suggested that star formation process peaked at z ~ 2-3 on the average. We use the stochastic self-propagating star formation model combined with gas infall from intergalactic medium to explore the parameter space in which the formations of the...
Main Authors: | Kui-Yun Huang, 黃癸雲 |
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Other Authors: | Wing-Huen Ip |
Format: | Others |
Language: | zh-TW |
Published: |
2002
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Online Access: | http://ndltd.ncl.edu.tw/handle/69219490557588710222 |
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