You are here: Home / Datasets (WP5,WP1) / Very Massive Star Models / Selected final structure for PCSNe studies

Selected final structure for PCSNe studies

Models studied in Whalen et al 2013 http://adsabs.harvard.edu/abs/2013arXiv1312.5360W + one extra model for comparison. Final model calculated is oxygen burning.
File Troff document P120z14S4.v0105241.out
File Troff document P150z02S4.v0056341.out
File Troff document P200z02S4.v0109321.out
File Troff document P300z02S4.v0064321.out
File Troff document P500z06S4.v0070921.out