The following digrams are done by reading the #presn file. In addition to the isotope abundances through the volume of the star (labelled), the following are also represented, but not labelled:

• Dark gray region: the "core". Here, the "core' is actually the part of the star below the piston (set at the bottom of the oxygen shell).
• Light gray regions: convective regions of the star's interior.
• Solid gray line: Nuclear energy generation rate.
• Dashed gray line: Density.

1. File s25_0520_0624:

2. File s25_0640_0768:

3. File s25_0760_0912:

4. File s25_0820_0984:

5. File s25_0880_1056:

6. File s25_0910_1092:

7. File s25_0940_1128:

8. File s25_0970_1164:

9. File s25_1000_1200:

10. File s25_1030_1236:

11. File s25_1060_1272:

12. File s25_1090_1308:

13. File s25_1120_1344:

14. File s25_1180_1416:

15. File s25_1240_1488:

16. File s25_1360_1632:

17. File s25_1480_1776:

18. File s25_1600_1920: