Table 2
Chemical composition of the stellar targets.
| Name | X0 | Z0 | Xsurf | Zsurf | (Z/X)surf | (Z/X)surf, ⊙ | |
|
|
|||||||
| Aardvark | 0.71550 | 0.01755 | 0.71543 | 0.01755 | 0.02453 | 0.0245 | |
| Blofeld | 0.71400 | 0.02000 | 0.78280 | 0.01579 | 0.02018 | 0.0165 | |
| Coco | 0.74140 | 0.00360 | 0.74132 | 0.00360 | 0.00486 | 0.0245 | |
| Diva | 0.72600 | 0.02600 | 0.72593 | 0.02600 | 0.03582 | 0.0245 | |
| Elvis | 0.71550 | 0.01755 | 0.71543 | 0.01755 | 0.02453 | 0.0245 | |
| Felix | 0.71550 | 0.01755 | 0.71543 | 0.01755 | 0.02453 | 0.0245 | |
| George | 0.71550 | 0.01755 | 0.71543 | 0.01755 | 0.02453 | 0.0245 | |
| Henry | 0.72600 | 0.01000 | 0.78010 | 0.00825 | 0.01058 | 0.0245 | |
| Izzy | 0.72600 | 0.01000 | 0.72593 | 0.01000 | 0.01378 | 0.0245 | |
| Jam | 0.71550 | 0.01755 | 0.71543 | 0.01755 | 0.02453 | 0.0245 | |
Notes. The last column specifies the reference solar value of (Z/X) used to obtain the value of [Fe/H]. Blofeld and Henry include atomic diffusion (see Table 3), thereby leading to different surface abundances. Even in the other models, the value of X decreases slightly due to deuterium burning.
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