V/R Variation of H-alpha Emition Lines for Be Stars : HR 6118, HR 6451, HR 8402, and HR 8628
The investigation of B Emission stars is mainly caused by the difference of characteristics among its members. This final project studies one of B Emission star variation in its double-peak emission line profile known as V/R (Violet/Red) variation. This variation illustrates intensity change from vi...
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Format: | Final Project |
Language: | Indonesia |
Online Access: | https://digilib.itb.ac.id/gdl/view/10938 |
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Institution: | Institut Teknologi Bandung |
Language: | Indonesia |
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