Figure 1
PNS recoil velocities as a function of time after the formation of the bounce shock. The subscript in the simulation names refers to the electron neutrino, , and anti-electron neutrino, , luminosities, each in units of 1052 erg sāˆ’1 (see equations 2 and 3 and Table 1).

PNS recoil velocities as a function of time after the formation of the bounce shock. The subscript in the simulation names refers to the electron neutrino, formula⁠, and anti-electron neutrino, formula⁠, luminosities, each in units of 1052 erg sāˆ’1 (see equations 2 and 3 and Table 1).

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