merger_2012_11+09

This is model merger_2012_11+09. Time at the end of this simulation: 100.07 s If you make use of the data provided through this website please cite the following paper(s): Pakmor, R., Kromer, M., Taubenberger, S., Sim, S. A., Röpke, F. K., & Hillebrandt, W. (2012): Normal Type Ia Supernovae from Violent Mergers of White Dwarf Binaries, The Astrophysical Journal Letters, 747, L10, ADS gamma ray data: Summa, A., Ulyanov, A., Kromer, M., Boyer, S., Röpke, F. K., Sim, S. A., Seitenzahl, I. R., Fink, M., Mannheim, K., Pakmor, R., Ciaraldi-Schoolmann, F., Diehl, R., Maeda, K., & Hillebrandt, W. (2013): Gamma-ray diagnostics of Type Ia supernovae. Predictions of observables from three-dimensional modeling, Astronomy and Astrophysics, 554, A67, ADS early light curve data: Noebauer, U. M., Kromer, M., Taubenberger, S., Baklanov, P., Blinnikov, S., Sorokina, E., & Hillebrandt, W. (2017): Early light curves for Type Ia supernova explosion models, Monthly Notices of the Royal Astronomical Society, 472, 2787, ADS Please also add the following acknowledgements: “This work made use of the Heidelberg Supernova Model Archive (HESMA), https://hesma.h-its.org”.

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merger_2012_11+09

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  • Date uploaded: Sept. 24, 2024, 11:07 a.m.
  • merger_2012_11+09
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