Searching for Be Stars in Open Clusters by using PTF Observations
碩士 === 國立中央大學 === 天文研究所 === 105 === A Be star is "a non-supergiant B star that has, or had at some time, one or more Balmer lines in emission". The Balmer emission lines are thought to originate from curcumstellar disks, but the formation and evolution of Be stars are still unclear. Theref...
| Main Authors: | , |
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| Other Authors: | |
| Format: | Others |
| Language: | zh-TW |
| Published: |
2017
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| Online Access: | http://ndltd.ncl.edu.tw/handle/7rpr8m |