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Table D.1.
Atmospheric parameters for S stars from S18, S19, and S20.
| Name | Teff | L | log g | [Fe/H] | σ[Fe/H] | C/O | [s/Fe] | Mcurr | Mini |
|---|---|---|---|---|---|---|---|---|---|
| (K) | (L⊙) | (M⊙) | (M⊙) | ||||||
| Tc-rich S stars from S18 | |||||||||
| V915 Aql | 3400 | 2000 | 0 | −0.50 | 0.15 | 0.75 | 0 | 0.8 | 1.0 |
| (3400; 3400) | (1900; 2000) | (0; 1) | (0.65; 0.75) | (0; 1) | |||||
| NQ Pup | 3700 | 2800 | 1 | −0.30 | 0.05 | 0.50 | 1 | 2.4 | 2.5 |
| (3500; 3700) | (2700; 2900) | (1; 2) | (0.5; 0.75) | (1; 1) | |||||
| UY Cen | 3300 | 11884 | 0 | −0.30 | 0.15 | 0.999 | 1 | 3.6 | 4.0 |
| (3000; 3400) | (11100; 13000) | (0; 3) | (0.971; 0.999) | (1; 2) | |||||
| Tc-rich S stars from S19 | |||||||||
| HD 357941 | 3400 | 8300 | 0 | −0.48 | 0.14 | 0.5 | 0 | 3.2 | 3.5 |
| (100; 100) | (7400; 9300) | (0; 1) | (0.5; 0.75) | (0; 1) | |||||
| CSS 154 | 3400 | 3000 | 1 | −0.29 | 0.20 | 0.5 | 0 | 1.4 | 1.6 |
| (100; 100) | (2700; 3300) | (1; 3) | (0.5; 0.899) | (0; 1) | |||||
| CSS 182 | 3500 | 2500 | 1 | −0.40 | 0.21 | 0.5 | 1 | 1.1 | 1.3 |
| (100; 100) | (2200; 2800) | (1; 3) | (0.5; 0.899) | (1; 1) | |||||
| CD −29°5912 | 3600 | 2700 | 1 | −0.40 | 0.22 | 0.5 | 1 | 1.3 | 1.5 |
| (100; 100) | (2500; 3000) | (1; 3) | (0.5; 0.899) | (1; 1) | |||||
| BD +34°1698 | 3400 | 3800 | 0 | −0.70 | 0.20 | 0.5 | 1 | 1.2 | 1.4 |
| (200; 200) | (3300; 4400) | (0; 3) | (0.5; 0.899) | (1; 1) | |||||
| Tc-rich S stars from S20 | |||||||||
| o1 Ori | 3500 | 3000 | 1 | −0.28 | 0.19 | 0.75 | 0 | 1.6 | 1.8 |
| (3500; 3600) | (2800; 3300) | (0; 2) | (0.5; 0.90) | (0; 1) | |||||
| BD +79 156 | 3600 | 2600 | 1 | −0.16 | 0.12 | 0.50 | 1 | 2 | 2.1 |
| (3600; 3700) | (2400; 2700) | (1; 3) | (0.50; 0.75) | (1; 1) | |||||
| Tc-poor S stars from S18 | |||||||||
| HD 189581 | 3500 | 1700 | 1 | 0.00 | 0.13 | 0.50 | 0 3 | 1.6 | 1.8 |
| (3500;3500) | (1600; 1800) | (1; 2) | (0.50; 0.75) | (0; 0) | |||||
| HD 233158 | 3600 | 1900 | 1 | −0.40 | 0.16 | 0.50 | 1 | 1.1 | 1.3 |
| (3600; 3600) | (1800; 2000) | (1; 1) | (0.50; 0.75) | (1; 1) | |||||
| HD 191589 | 3700 | 500 | 1 | −0.30 | 0.10 | 0.75 | 1 | 1 | 1 |
| (3700; 3800) | (500; 600) | (1; 2) | (0.75;0.75) | (1; 1) | |||||
| HD 191226 | 3600 | 6400 | 1 | −0.10 | 0.13 | 0.75 | 1 | 4.6 | 5.0 |
| (3600; 3600) | (6100; 6800) | (0; 1) | (0.50; 0.899) | (1; 1) | |||||
| V530 Lyr | 3500 | 1700 | 1 | 0.00 | 0.10 | 0.50 | 1 | 1.6 | 1.8 |
| (3500; 3600) | (1600; 1800) | (1; 3) | (0.50; 0.75) | (1; 1) | |||||
| HD 215336 | 3700 | 600 | 1 | 0.00 | 0.12 | 0.50 | 1 | 1.0 | 1.2 |
| (3700; 3700) | (500; 600) | (1; 1) | (0.50; 0.75) | (1; 1) | |||||
| HD 150922 | 3600 | 5000 | 0 | −0.50 | 0.12 | 0.50 | 1 | 2.1 | 2.2 |
| (3600; 3600) | (4800; 5100) | (0; 1) | (0.50; 0.75) | (1; 1) | |||||
| HD 63733 | 3700 | 1500 | 1 | −0.10 | 0.13 | 0.50 | 1 | 2.2 | 2.3 |
| (3700; 3700) | (1400; 1600) | (1; 2) | (0.50; 0.75) | (1; 1) | |||||
| BD +69°524 | 3600 | 900 | 1 | −0.40 | 0.11 | 0.50 | 0 | 1.0 | 1.0 |
| (3600; 3600) | (800; 900) | (1; 2) | (0.50; 0.75) | (0; 0) | |||||
| BD +28°4592 | 3700 | 600 | 1 | −0.10 | 0.12 | 0.75 | 1 | 1.1 | 1.3 |
| (3700; 3800) | (600; 700) | (1; 2) | (0.50; 0.899) | (1; 1) | |||||
| V1135 Tau | 3400 | 1700 | 1 | −0.20 | 0.14 | 0.50 | 1 | 1.0 | 1.2 |
| (3400; 3500) | (1600; 1800) | (0; 1) | (0.5; 0.951) | (1; 1) | |||||
| AB Col | 3500 | 2000 | 1 | 0.00 | 0.14 | 0.50 | 1 | 1.9 | 2.0 |
| (3300; 3500) | (1900; 2000) | (1; 2) | (0.50; 0.75) | (1; 1) | |||||
| TYC 5971-534-1 | 3600 | 800 | 1 | −0.10 | 0.18 | 0.899 | 1 | 1.1 | 1.3 |
| (3600; 3600) | (700; 900) | (0; 2) | (0.50; 0.899) | (1; 2) | |||||
| BD −10°1977 | 3500 | 6100 | 0 | −0.50 | 0.15 | 0.50 | 1 | 1.5 | 1.7 |
| (3500; 3600) | (5700; 6500) | (0; 1) | (0.50; 0.899) | (1; 1) | |||||
| FX CMa | 3500 | 6500 | 1 | 0.00 | 0.14 | 0.971 | 1 | 4.2 | 4.5 |
| (3500; 3500) | (6100; 7100) | (1; 1) | (0.951; 0.971) | (1; 1) | |||||
| BD −22°1742 | 4000 | 600 | 1 | −0.30 | 0.09 | 0.75 | 0 | 1.5 | 1.7 |
| (4000; 4000) | (500; 600) | (1; 5) | (0.50; 0.899) | (0; 1) | |||||
Notes. The L column indicates the luminosity and its error due to the Gaia EDR3 error on the parallax. All the other columns are the same as in Table 3.
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