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...

Full description

Bibliographic Details
Main Authors: Kui-Yun Huang, 黃癸雲
Other Authors: Wing-Huen Ip
Format: Others
Language:zh-TW
Published: 2002
Online Access:http://ndltd.ncl.edu.tw/handle/69219490557588710222