Spiral Density Waves in a Gas Disk of Rigid-body Rotation

碩士 === 國立中央大學 === 天文研究所 === 89 === The observed rotation laws near the center $(<1 kpc)$ for almost all nearby spiral galaxies can be approximated by a rigid-body rotation. The density-wave theory of galactic spirals is tailored to handling a differenti...

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Bibliographic Details
Main Authors: Mei-Yin Chou, 周美吟
Other Authors: Prof. Chih-Kang Chou
Format: Others
Language:en_US
Published: 2001
Online Access:http://ndltd.ncl.edu.tw/handle/34758723470617613593