Fig. 6.
Density and velocity profile of the SGRB ambient medium model. The red line shows a snapshot of the density profile (along the polar axis) of the neutron star merger ejecta model described in Xie et al. (2018) (also used in Kasliwal et al. 2017 and Gottlieb et al. 2018b). The blue dashed line shows the corresponding velocity profile (velocity axis on the right). The ejecta are assumed to expand homologously.
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