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Representative Trajectories of a magneto-rotational supernova

Representative trajectories for the MR-SN model 35OC-Rs (Obergaulinger & Aloy, MNRAS, 469, L43, 2017) and their nucleosynthesis (Reichert et al., MNRAS, 501, 5733, 2021).

If you use the trajectories (tracer_x.dat) or nucleosynthesis output (finab.dat), please cite both papers:

  • Obergaulinger & Aloy, MNRAS, 469, L43 (2017)
  • Reichert et al., MNRAS, 501, 5733, (2021)

The trajectories are separate into different groups as described in Reichert et al. (2020). For each group, ten representative trajectories are given, which have been selected so that on average they best match the integrated pattern of all trajectories in that group. The ejected mass within of each group is given in the following table:

Group Mass [M sol]
Alpha 0.11559
Alpha-Fe 0.04133
Fe 0.06586
Fe-weak-r 0.11259
Weak-r 0.04156
r-process 0.01207
Total 0.38900

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