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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Bibliographic Details
Main Author: GIOVANY (NIM: 103 04 007), MONALIZA
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