Fig. 2.

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Effect of different explosion energies and prescriptions on three representative p-nuclei. Left panels: 92Mo (upper panel), 130Ba (central panel), and 196Hg (lower panel) abundances in mass fractions as a function of the internal mass coordinate (solid lines, left axis) and explosion peak temperature in T9 (dashed lines, right y-axis) in the 20 M⊙ SBW models. Different colors denote different shock velocities. Right panels: same as the left panels but for a sample of the 15 M⊙ LAW models, without the explosion peak temperature plotted. The horizontal dashed-dotted blue line in each panel represents the solar abundance of the representative isotope in mass fractions taken from Asplund et al. (2009).
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