Fig. 2.
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Mass of the dynamical ejecta (left), velocity of the dynamical ejecta (centre), and mass of the disc (right) for the EOS BLh, as defined in Eqs. (6)–(8). x and y axes represent the masses M1 and M2 of the BNS. The solid and the dashed black lines mark the chirp mass of GW170817 and GW190425, respectively. Triangular markers show the prompt-collapse mass threshold MPC.
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