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Table 6.
Comparison with carbon star observations.
| star | ω = 0.10 | ω = 0.12 | ω = 0.14 | Tc | Mbol |
|---|---|---|---|---|---|
| AW Cyg | 0.05 | 0.05 | 0.05 | Y | −5.7 |
| S Sct | 0.13 | 0.13 | 0.12 | Y | −4.6 |
| SS Vir | 0.02 | 0.02 | 0.02 | D | ... |
| SZ Sgr | 0.07 | 0.04 | 0.02 | D | −2.1 |
| U Hya | 0.21 | 0.14 | 0.10 | Y | −4.0 |
| V460 Cyg | 0.03 | 0.01 | 0.01 | Y | −5.8 |
| Z Psc | 0.18 | 0.11 | 0.07 | Y | −4.1 |
| Total | 0.69 | 0.50 | 0.39 | ||
Notes. L2-averaged errors between the abundances observed in solar metallicity C-rich AGB stars (Abia et al. 2001, 2002) and the best fitting model in each simulation. The Tc column indicates Tc detection (Y) or doubtful detection (D).
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