ANALISIS VARIASI V/R GARIS EMISI H? BERDASARKAN PARAMETER FISIS SPEKTRUM PADA BINTANG B- EMISI EW LAC
B-emission (Be) stars are non-supergiant B-type stars whose spectra have, or have had at some time, one or more Balmer lines in emission. Be stars usually have variability on their spectra emission and the variability varies differently on each star. EW Lacertae (HR 8731) is one of B-emission stars...
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| Format: | Theses |
| Language: | Indonesia |
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| Online Access: | https://digilib.itb.ac.id/gdl/view/61144 |
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| Institution: | Institut Teknologi Bandung |
| Language: | Indonesia |