The following digrams are done by reading the #presn file. The x-axis has been cut off at 5, 7 and 9 solar masses for the 15, 20 and 25 solar mass stars respectively in order to see more clearly what happens below these mass limits. 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". The "core' is the ACTUAL iron core (given by: (value of parameter 61 in D#final file) / (1.98892 x 10^33)).
• Light gray regions: convective regions of the star's interior.
• Solid gray line: Nuclear energy generation rate.
• Dashed gray line: Density.

1. File s25_0760_1200:

2. File s25_0820_1200:

3. File s25_0880_1200:

4. File s25_0940_1200:

5. File s25_1000_1200:

6. File s25_1060_1200:

7. File s25_1120_1200:

8. File s25_1180_1200:

9. File s25_1240_1200: