Very massive stars : mass determination and fate / Norhasliza binti Yusof
The first generation of stars is thought to have been very massive (150-300 M�) and produces pair creation supernovae (PCSNe) at the end of their life. However, the chemical signature of PCSNe is not observed in extremely metal poor stars (e.g. Umeda & Nomoto, 2002) and it raises the followin...
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| Format: | Thesis |
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2012
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| Online Access: | http://studentsrepo.um.edu.my/4555/1/Norhasliza_PhD_tesis.pdf http://studentsrepo.um.edu.my/4555/ |
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