Interaction of Magnetic Fields and Kinematics in Star-forming Regions from Parsec-scale Filaments to Thousand-AU-scale Cores
博士 === 國立清華大學 === 天文研究所 === 105 === Star formation takes place in the high-density regions of molecular clouds where magnetic fields and turbulence are the two main mechanism support- ing molecular clouds against self-gravity. Recent observations of molecular clouds reveal a two-step scenario of sta...
| Main Authors: | , |
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| Other Authors: | |
| Format: | Others |
| Language: | en_US |
| Published: |
2017
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| Online Access: | http://ndltd.ncl.edu.tw/handle/2ry3ke |