Table 5.
Stellar parameters predicted by the FUNS code and from the HR diagram analysis of the OCs for the stars in the sample.
| Star | Cluster | Mstar | Mbol | [M/H] | TDU | Mcore | Mto | Mfinal | log (age) |
|---|---|---|---|---|---|---|---|---|---|
| (M⊙) | (mag) | (dex) | (M⊙) | (M⊙) | (M⊙) | (a) | |||
| Case 63 | Berkeley 9 | 1.80 | −4.67 | −0.10 | 3 | 0.585 | 1.75±0.25 | 0.620 | 9.25±0.19 |
| HD 292921 | Berkeley 34 | 1.50 | −4.54 | −0.19 | 2 | 0.578 | 1.65±0.35 | 0.630 | 9.33±0.23 |
| Case 473 | Berkeley 53 | 1.50 | −4.75 | 0.12 | 7 | 0.590 | 1.50±0.20 | 0.632 | 9.51±0.04 |
| Case 121 | Berkeley 72 | 2.00 | −4.70 | −0.18 | 4 | 0.587 | 2.25±0.25 | 0.634 | 8.97±0.10 |
| Case 588 | Dias 2 | 1.30 | −4.80 | −0.90 | 5 | 0.600 | 1.30±0.20 | 0.635 | 9.52±0.04 |
| IRAS 19582+2907 | FSR 0172 | 3.00 | −5.10 | 0.00 | 7 | 0.625 | 3.25±0.75 | 0.723 | 8.59±0.30 |
| HD 11800 | NGC 743 | 5.00 | −4.51 | 0.00 | e-AGB | 0.635 | 5.00±1.00 | 0.873 | 8.06±0.23 |
| [D75b] Star30 | NGC 1798 | 2.50 | −4.70 | 0.00 | 4 | 0.616 | 2.00±0.50 | 0.628 | 9.21±0.23 |
| BD +60 2534 | NGC 7654 | 6.00 | −4.50 | 0.00 | e-AGB | 0.707 | 5.00±1.00 | 0.873 | 8.06±0.23 |
| MSB 75 | NGC 7789 | 1.50 | −4.80 | −0.27 | 4 | 0.590 | 1.75±0.25 | 0.635 | 9.25±0.15 |
| C* 908 | Ruprecht 37 | 1.30 | −4.63 | −0.40 | 2 | 0.590 | 1.40±0.10 | 0.632 | 9.47±0.10 |
| CSS 0291 | Tombaugh 1 | 2.00 | −4.50 | −0.17 | 2 | 0.582 | 1.75±0.25 | 0.631 | 9.31±0.25 |
Notes. Mcore is the current core mass at the specified luminosity. The theoretical Mbol and [M/H] values should be compared with those determined observationally in Table 4 (column 5) and Table 3 (column 4), respectively. Column 6 indicates the number of TDUs episodes in the theoretical model during the TP-AGB phase for which we find agreement between the observed and predicted abundances according to the FRUITY database (see text).
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