ddt_2014_rpc32_ddt8_n100

This is model ddt_2014_rpc32_ddt8_n100. Time at the end of this simulation: 100.16 s If you make use of the data provided through this website please cite the following paper(s): Ohlmann, S. T., Kromer, M., Fink, M., Pakmor, R., Seitenzahl, I. R., Sim, S. A., & Röpke, F. K. (2014): The white dwarf’s carbon fraction as a secondary parameter of Type Ia supernovae, Astronomy and Astrophysics, 572, A57, ADS Please also add the following acknowledgements: “This work made use of the Heidelberg Supernova Model Archive (HESMA), https://hesma.h-its.org”.ddt_2014_c50_ddt8_n100