STUDI MORFOKINEMATIKA PLANETARY NEBULA SH 2-71 DENGAN PEMODELAN 3-D
A planetary nebula is formed when a low to intermediate mass star approaches the end of its life. Before the ejected materials finally being one with the insterstellar matters, a nebula will be visible surrounding its former stellar core. The variety of planetary nebulae visual appearances indic...
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| Format: | Final Project |
| Language: | Indonesia |
| Online Access: | https://digilib.itb.ac.id/gdl/view/57077 |
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| Institution: | Institut Teknologi Bandung |
| Language: | Indonesia |