Free Access

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

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.