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Table 2
Summary of ejecta properties used as initial conditions for the cmfgen calculations.
| Model | Mr | Me | Ekin | ⟨ Vm ⟩ | He | C | O | Si | Ca | 56Ni |
| [M⊙] | [M⊙] | [1051 erg] | [km s-1] | [M⊙] | [M⊙] | [M⊙] | [M⊙] | [M⊙] | [M⊙] | |
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| r0e2 | 1.71 | 9.69 | 4.12 | 6530 | 0.181 | 1.326 | 5.471 | 0.112 | 0.0061 | 0.122 |
| r0e4 | 1.54 | 9.86 | 12.31 | 11210 | 0.205 | 1.298 | 5.590 | 0.181 | 0.0098 | 0.172 |
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| r4e4 | 1.88 | 8.12 | 13.44 | 12900 | 0.286 | 1.302 | 3.852 | 0.458 | 0.0410 | 0.583 |
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| r6e4 | 1.62 | 4.97 | 12.41 | 15840 | 0.324 | 1.051 | 2.072 | 0.315 | 0.022 | 0.300 |
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| r6ze4 | 1.99 | 7.70 | 13.70 | 13370 | 1.453 | 0.822 | 3.017 | 0.429 | 0.0386 | 0.696 |
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| r6e4BH | 4.04 | 2.55 | 11.63 | 21420 | 0.456 | 0.910 | 0.515 | 0.051 | 0.0036 | 0.435 |
Notes. All models derive from pre-SN mesa models named r0, r4, r6, or r6z (see Table 1). Model r6e4BH forms a 4.04 M⊙ BH – all other models leave behind a 1.6–1.9 M⊙ neutron star.
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