Table 1
Transition mass and properties for different chemistries.
| Y | M/M⊙ | Teff | log(L/L⊙) | mF322W2 | mF115W - mF322W2 | mF150W2 - mF322W2 |
|---|---|---|---|---|---|---|
| 1G, Y = 0.255 | 0.074 | 1581 | −4.39 | 12.10 | 1.95 | 1.25 |
| 2G, Y = 0.28 | 0.073 | 1701 | −4.26 | 11.75 | 2.06 | 1.31 |
| 2G, Y = 0.30 | 0.071 | 1712 | −4.29 | 11.79 | 2.11 | 1.34 |
| 2G, Y = 0.35 | 0.066 | 1630 | −4.37 | 11.89 | 2.24 | 1.4 |
Notes. The table lists various theoretical and observational properties of stellar models of minimum mass that reach Lpp = Lnuc at the age of 12 Gyr, for different chemical compositions. Column 1 gives the helium content and if the composition refers to 1G or 2G, Cols. 2 and 3 give Teff and luminosity, whereas Cols. 3-6 report Mf322w2 and the (mF115W - mF322W2) and (mF150W - mF322W2) colours.
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