Table 1.
Summary of ejecta properties used as initial conditions for our dust calculations. (See Sect. 2 for discussion).
Model | Age | Mej | Ekin | M(O) | M(56Ni) | Ldecay,abs | Lsh,abs | VCDS | MCDS |
---|---|---|---|---|---|---|---|---|---|
[d] | [M⊙] | [erg] | [M⊙] | [M⊙] | [erg s−1] | [erg s−1] | [km s−1] | [M⊙] | |
SN IIn | 300 | 12.00 | 1.5(51) | 0.75 | 0.032 | 3.1(40) | 2.0(41) | 5000 | 2.4 |
SN IIP/CSM | 1000 | 11.49 | 9.2(50) | 1.02 | 0.063 | 3.2(37) | 1.0(40) | 8000 | 0.13 |
SN II | 700 | 11.36 | 9.2(50) | 1.02 | 0.063 | 8.3(38) | … | … | … |
Notes. The columns give the age, the total mass, the kinetic energy, the O and 56Ni mass for each ejecta model. We then give the absorbed decay power in each model, and for the SN IIn and SN IIP/CSM, we also give the total shock power absorbed in the outer ejecta dense shell, whose velocity and mass are given in the last two columns. In the SN II model, the only power source is radioactive decay. Numbers in parentheses refer to powers of ten.
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