Published October 19, 2021
| Version 1
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Late-time spectral line formation in Type IIb supernovae, with application to SN 1993J, SN 2008ax, and SN 2011dh
Description
Spectral models for stripped cores of M_ZAMS=12, 13, 17 Msun progenitors, 100-500d. Distance 7.8 Mpc assumed.
Files
Files
(3.2 MB)
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md5:e7411f7b319f568cde9d69f69ac09e77
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3.2 MB | Download |
Additional details
Related works
- Is documented by
- Journal article: 10.1051/0004-6361/201423983 (DOI)