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Fig. 2.


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Evolution of different quantities of our model. Lower panel: Kippenhahn diagram showing the convective zones dashed in black, and the neutron density in cm−3 color-coded in shades of blue. The x-axis shows the time in years measured since the maximum release of energy of the He flash. The y-axis shows the outer mass in logarithmic scale, ln(1 − mr/M), being mr the mass coordinate and M = 0.4846 M the mass of the star after the stripping. Upper panel: evolution of the luminosity due to He- (blue line) H-burning (orange line), respectively, and of the maximum value of the neutron density (red dashed line).

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