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Fig. 4.

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Compositions and evolutionary stages of our SERIES I models when calculations were terminated, in raster format. Metallicity for the bottom, middle, and top panel is Z = 10−4, Z = 10−3, and Z = 0.02 respectively, while the colorbar indicates the composition of the core at the endpoint of the simulation (see text). Semihatched regions show models that stopped only after developing a near-MCh core within the range 1.35−1.37 M, shortly before oxygen ignition. All these models also have no envelopes and contain no helium. Fully hatched regions show models with near-MCh cores that reached the explosive oxygen burning stage. All nonhatched ONe models stopped before their entire envelope was lost, and have cores with masses between (1.0 < Mc/M ≤ 1.36).

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