PUSHing Core-collapse Supernovae to Explosions in Spherical Symmetry. II. Explodability and Remnant Properties

@article{Ebinger2018PUSHingCS,
  title={PUSHing Core-collapse Supernovae to Explosions in Spherical Symmetry. II. Explodability and Remnant Properties},
  author={K. Ebinger and S. Curtis and C. Frohlich and M. Hempel and A. Perego and M. Liebendorfer and Friedrich-Karl Thielemann},
  journal={The Astrophysical Journal},
  year={2018},
  volume={870},
  pages={1}
}
In a previously presented proof-of-principle study we established a parametrized spherically symmetric explosion method (PUSH) that can reproduce many features of core-collapse supernovae. The present paper goes beyond a specific application that is able to reproduce observational properties of SN1987A and performs a systematic study of the explosion properties for an extensive set of non-rotating, solar metallicity stellar progenitor models in the mass range from 10.8 to 120 M$_\odot$.This… Expand
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