A comparison between the production factor plots is done between 2 studies: one using the Anders & Grevess 1989 solar abundances (the present study) and the other making use of the Lodders 2004 solar abundances (previous study) for the initial composition of the masive stars being considered.
| 1. 3 star average (15, 20, 25 Msun) (Boyes et al. medium weight elements) | |
| a). AG89 | b). Lodders04 |
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2. 3 star average (15, 20, 25 Msun) (all medium weight elements) |
| a). AG89 | b). Lodders04 |
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3. 2 star average (15, 25 Msun) (Boyes et al. medium weight elements) |
| a). AG89 | b). Lodders04 |
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4. 2 star average (15, 25 Msun) (all medium weight elements) |
| a). AG89 | b). Lodders04 |
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| 5. 9 star average (13, 15, 17, 19, 20, 21, 23, 25, 27 Msun) (Boyes et al. medium weight elements) | |
| a). AG89 | |
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| 6. 9 star average (13, 15, 17, 19, 20, 21, 23, 25, 27 Msun) (all medium weight elements) | |
| a). AG89 | |
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| 7. odd star average (13, 15, 17, 19, 21, 23, 25, 27 Msun) (Boyes et al. medium weight elements) | |
| a). AG89 | |
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| 8. odd star average (13, 15, 17, 19, 21, 23, 25, 27 Msun) (all medium weight elements) | |
| a). AG89 | |
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