Spectral modeling of nebular-phase supernovae
Massive stars live fast and die young. They shine furiously for a few million years, during which time they synthesize most of the heavy elements in the universe in their cores. They end by blowing themselves up in a powerful explosion known as a supernova (SN). During this process, the core collaps...
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| Format: | Doctoral Thesis |
| Language: | English |
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Stockholms universitet, Institutionen för astronomi
2011
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| Online Access: | http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-64130 http://nbn-resolving.de/urn:isbn:978-91-7447-407-7 |