#TITLE_ALTERNATIVE#
B-emission (Be) stars are B-type stars class with luminosity III – V, rotate very fast and show the emission profile of the hydrogen Balmer line, especially Hα. The existence of emission lines in the visual region, shows that here is a cold envelope around the star’s equator. Observat...
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| Format: | Final Project |
| Language: | Indonesia |
| Online Access: | https://digilib.itb.ac.id/gdl/view/30089 |
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| Institution: | Institut Teknologi Bandung |
| Language: | Indonesia |