Identification of Herbig Ae/Be Stars in Open Clusters
碩士 === 國立中央大學 === 天文研究所 === 94 === Herbig Ae/Be stars are intermediate-mass young stars. The fast evolution in the premain sequence phase causes a much less number of-and hence relatively poorer knowledge toward|Herbig Ae/Be stars than that of low-mass young stars. In addition to the emission lines...
| Main Authors: | , |
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| Format: | Others |
| Language: | zh-TW |
| Online Access: | http://ndltd.ncl.edu.tw/handle/d8dqm4 |