ddt_2014_c50_ddt8_n100

This is model ddt_2014_c50_ddt8_n100. Time at the end of this simulation: 100.23 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”.

Reference: https://ui.adsabs.harvard.edu/abs/2014A%26A...572A..57O/abstract
Date uploaded: Sept. 24, 2024, 7:17 a.m.
Author: Ohlmann et al.
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