ANALISIS VARIASI SPEKTRUM GARIS H-ALFA BINTANG B-EMISI PADA BERBAGAI SUB KELAS SPEKTRUM B
Be stars are non-giant spectral class B stars that have or are currently having emission lines in their spectrum. The selected object was based on a paper from Slettebak, et al (1992) which amounted to 41 program stars. However, there is 1 star program, namely HD 68980 which does not have good...
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| Format: | Final Project |
| Language: | Indonesia |
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| Online Access: | https://digilib.itb.ac.id/gdl/view/55267 |
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| Institution: | Institut Teknologi Bandung |
| Language: | Indonesia |