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...
Saved in:
| Main Author: | |
|---|---|
| Format: | Thesis |
| Published: |
2012
|
| Subjects: | |
| Online Access: | http://studentsrepo.um.edu.my/4555/1/Norhasliza_PhD_tesis.pdf http://studentsrepo.um.edu.my/4555/ |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|