#TITLE_ALTERNATIVE#
Nonradial pulsation is generally occurred on stars, including intermediate-mass stars. Pulsating intermediate-mass stars can be represented by 𝛽 Cephei and SPB (slowly pulsating B) type, whose pulsations are dominantly characterized respectively as p-mode and g-mode. In this study, the p...
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| Format: | Final Project |
| Language: | Indonesia |
| Online Access: | https://digilib.itb.ac.id/gdl/view/20240 |
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| Institution: | Institut Teknologi Bandung |
| Language: | Indonesia |
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