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- W2955907595 abstract "We apply the parametrized, spherically symmetric explosion method PUSH to two sets of pre-explosion models suitable for SN 1987A: blue supergiants (BSGs) resulting from the merger of a main sequence star with a giant and red supergiants (RSGs) representing the end point of single-star stellar evolution. For each model, we perform a calibration of the PUSH method to the observational properties of SN 1987A and calculate the detailed explosive nucleosynthesis yields. We find that such a calibration to SN 1987A is only possible for one of the BSG models. We compare the yields from this model with the yields from the best-fit RSG model. The largest differences are found for nuclei in the mass range of 20 ≤ A ≤ 40 which are mostly synthesized pre-explosion. We predict a neutron star with a gravitational mass of 1.48 M ⊙ from the BSG model and a neutron star of 1.41 M ⊙ from the RSG model." @default.
- W2955907595 created "2019-07-12" @default.
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- W2955907595 date "2019-07-02" @default.
- W2955907595 modified "2023-10-01" @default.
- W2955907595 title "Nucleosynthesis for SN 1987A from single-star and binary-merger progenitors" @default.
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- W2955907595 doi "https://doi.org/10.1088/1361-6471/ab1ff7" @default.
- W2955907595 hasPublicationYear "2019" @default.
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