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Table 1.
Assumed ejecta properties for NSNS and BHNS mergers.
Parameter | Description | NSNS | BHNS |
---|---|---|---|
ξw | Accretion disc mass fraction flowing in wind ejecta | 0.05 | 0.01 |
ξs | Accretion disc mass fraction flowing in secular ejecta | 0.2 | 0.2 |
vw | Wind ejecta velocity | 0.1 c | 0.1 c |
vs | Secular ejecta velocity | 0.1 c | 0.1 c |
kd | Dynamical ejecta opacity | 15 cm2 g−1 | 15 cm2 g−1 |
kw | Wind ejecta opacity | 0.5 cm2 g−1 | 1 cm2 g−1 |
ks | Secular ejecta opacity | 5 cm2 g−1 | 5 cm2 g−1 |
θd | Dynamical ejecta latitudinal opening angle (from the equatorial plane) | 80 deg | 17 deg |
ϕd | Dynamical ejecta azimuthal opening angle | 2π rad | π rad |
θw | Wind ejecta opening angle (from the polar axis) | 60 deg | 60 deg |
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