Evolution in the Tc−ρc-diagram for the three stellar models at Z = Z⊙/ 50 (with the masses at helium depletion as indicated) calculated to the final evolutionary stage. The shaded region shows the region that is unstable to pair creation. Both the 35 M⊙ and the 200 M⊙ stars collapse to form black holes, while the 90 M⊙ is disrupted in a PISN.
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