Nebular-phase spectra (MZAMS=12, 13, 17 Msun, t=100-500d) for Type IIb SNe were published by Jerkstrand, Ergon, Smartt, Fransson, Sollerman, Taubenberger, Bersten, Spyromilio 2015, A&A.

The models are available here. There is a neglegible influence of the hydrogen envelope after ~150 days in these models, which means they can be compared to Type Ib SNe as well after that time.

A IIb model was also presented in Maurer+2011.

users/ajerkstrand/iib.txt · Last modified: 2016/03/30 13:36 by Anders Jerkstrand

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