Near Infrared Excess of Classical Be star
碩士 === 國立中央大學 === 天文研究所 === 97 === Classical Be stars are B-type main sequence stars with one or more Balmer lines in emission, characterized by their rotational velocity (up to 300 km s−1), and circumstellar gas distributed in shell-, disk- or ring like configuration. Classical Be stars also are...
| Main Authors: | , |
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| Format: | Others |
| Language: | en_US |
| Online Access: | http://ndltd.ncl.edu.tw/handle/9s3gse |