Fig. 5.
Light curves for the same neutron star model and outburst model as in Fig. 2, computed for either fully accreted crust (solid and dot-dashed lines) or partially accreted crust with replaced matter filling the layer up to ρacc = 5 × 1010 g cm−3 (dashed and dotted lines) for models HZ’08 (solid and dashed lines) and F+18 (dot-dashed and dotted lines), as shown in the legend.
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