Table A.1.
Chemical data and depletion profiles.
| Star name | Teff (K) | [Fe/H] | [Zn/Ti] | [S/Ti] | [Zn/Fe] | Depletion profile | Tturn − off (K) | Reference |
|---|---|---|---|---|---|---|---|---|
| 89 Her | 6600 | −0.5 | 0.6 | 0.7 | 0.1 | S | 1500 | 1 |
| AC Her | 5800 | −1.5 | 1.0 | 1.2 | 0.7 | U | 1200 | 2, 3 |
| AD Aql | 6300 | −2.1 | 2.5 | 2.6 | 2.0 | S | 1000 | 3 |
| AI Sco | 5300 | −0.7 | 0.3 | 0.8 | 0.1 | P | 1100 | 4 |
| AR Pup | 6000 | −0.9 | / | 2.6 | / | S | 1200 | 5 |
| AZ Sgr | 4750 | −1.6 | / | 1.2 | / | P | 1000 | 4 |
| BD+39 4926 | 7750 | −2.4 | 2.0 | 2.8 | 1.7 | S | 1000 | 6 |
| BD+46 442 | 6250 | −0.8 | −0.2 | 0.2 | 0.0 | N | / | 7, 8 |
| BT Lac | 5000 | −0.2 | 0.5 | / | 0.1 | S | 1400 | 7 |
| BZ Sct | 6250 | −0.8 | 1.3 | 1.4 | 0.9 | S | 1000 | 4 |
| CC Lyr | 6250 | −3.6 | / | / | 3.0 | S | 1000 | 9 |
| CT Ori | 5700 | −1.9 | 1.9 | 2.0 | 1.3 | S | 1200 | 10 |
| DF Cyg | 4800 | 0.0 | −0.7 | / | −0.6 | N | / | 4 |
| DY Ori | 5900 | −2.2 | 2.1 | 2.5 | 2.0 | U | 1000 | 4, 5 |
| EP Lyr | 6200 | −1.8 | 1.3 | 1.4 | 1.1 | P | 800 | 5 |
| EQ Cas | 4900 | −0.8 | 0.9 | 0.9 | 0.4 | S | 1500 | 4 |
| GK Car | 5500 | −1.3 | 1.2 | 1.5 | 0.9 | U | 1000 | 11 |
| GP Cha | 5500 | −0.6 | 0.0 | 0.3 | −0.1 | N | / | 12 |
| GZ Nor | 4875 | −2.1 | 0.8 | 1.5 | 1.0 | P | 800 | 11 |
| HD 108015 | 7000 | −0.1 | 0.1 | 0.1 | −0.1 | N | / | 13 |
| HD 131356 | 6000 | 0.0 | 0.55 | 0.5 | 0.2 | U | 1300 | 13 |
| HD 158616 | 7250 | −0.6 | 0.0 | 0.1 | 0.2 | N | / | 13, 14 |
| HD 213985 | 8200 | −0.9 | / | 1.9 | / | S | 1000 | 15 |
| HD 44179 | 7500 | −3.3 | / | / | 2.7 | U | 1000 | 15, 16 |
| HD 46703 | 6250 | −1.7 | 0.9 | 1.1 | 0.8 | P | 800 | 17 |
| HD 52961 | 6000 | −4.5 | 3.0 | 3.4 | 3.3 | U | 1100 | 7, 18, 19 |
| HP Lyr | 6300 | −1.0 | 2.6 | 3.0 | 0.6 | S | 1300 | 4 |
| HR 4049 | 7600 | −4.8 | / | / | 3.5 | S | 800 | 15 |
| IRAS 06165+3158 | 4250 | −0.9 | 0.0 | / | −0.1 | N | / | 7 |
| IRAS 08544−4431 | 7250 | −0.3 | 0.9 | 1.0 | 0.4 | S | 1200 | 20 |
| IRAS 09060−2807 | 6500 | −0.7 | 0.2 | 0.0 | 0.1 | N | / | 12 |
| IRAS 09144−4933 | 5750 | −0.3 | / | 1.3 | / | S | 1400 | 12 |
| IRAS 11472−0800 | 5750 | −2.7 | 3.4 | 3.8 | 1.8 | S | 1000 | 21 |
| IRAS 15469−5311 | 7500 | 0.0 | 1.8 | 2.1 | 0.3 | S | 1300 | 12 |
| IRAS 16230−3410 | 6250 | −0.7 | 1.0 | 1.1 | 0.3 | S | 1500 | 12 |
| IRAS 17038−4815 | 4750 | −1.5 | 0.7 | / | 0.3 | S | 1400 | 12 |
| IRAS 17233−4330 | 6250 | −1.0 | 1.4 | 1.8 | 0.7 | S | 1000 | 12 |
| IRAS 19125+0343 | 7750 | −0.3 | 2.3 | 2.6 | 0.4 | S | 1400 | 12 |
| IRAS 19135+3937 | 6000 | −1.0 | 0.5 | 0.8 | 0.0 | S | 1500 | 7 |
| IRAS 19157−0247 | 7750 | 0.1 | / | 0.4 | / | U | 1500 | 12 |
| IW Car | 6700 | −1.1 | 2.1 | 2.5 | 1.0 | S | 1100 | 22 |
| LR Sco | 5750 | −0.1 | 0.8 | 0.9 | 0.1 | S | 1400 | 4, 12 |
| QY Sge | 5850 | −0.3 | 1.2 | 1.2 | 0.1 | S | 1500 | 12 |
| R Sct | 4500 | −0.4 | 0.2 | / | 0.2 | N | / | 23 |
| R Sge | 5000 | −0.5 | 1.1 | 1.7 | 0.3 | S | 1200 | 5 |
| RU Cen | 6000 | −1.9 | 1.0 | 1.3 | 0.9 | P | 800 | 24 |
| RV Tau | 4500 | −0.4 | 0.5 | / | 0.4 | P | 1100 | 23 |
| SAO 173329 | 7000 | −0.8 | −0.1 | 0.0 | 0.0 | N | / | 6, 13 |
| SS Gem | 5400 | −0.9 | 2.0 | 1.6 | 0.9 | S | 1100 | 10 |
| ST Pup | 5500 | −1.5 | 2.1 | 2.0 | 1.4 | S | 800 | 25 |
| SU Gem | 5250 | −0.3 | 0.5 | 0.8 | 0.1 | S | 1400 | 7 |
| SX Cen | 6250 | −1.1 | 1.5 | 1.9 | 0.6 | S | 1100 | 24 |
| SZ Mon | 4700 | −0.4 | 0.8 | 1.5 | 0.0 | S | 1500 | 9 |
| TW Cam | 4800 | −0.5 | 0.3 | 0.6 | 0.1 | P | 1100 | 23 |
| U Mon | 5000 | −0.8 | 0.0 | 0.5 | 0.1 | N | / | 23 |
| UY Ara | 5500 | −1.0 | 1.4 | 1.7 | 0.7 | S | 1000 | 23 |
| UY CMa | 5500 | −1.3 | 1.8 | 2.1 | 0.7 | S | 1000 | 4 |
| V Vul | 4500 | −0.4 | −0.1 | 0.7 | 0.1 | N | / | 4 |
References.
(1) Kipper (2011); (2) Van Winckel et al. (1998); (3) Giridhar et al. (1998); (4) Giridhar et al. (2005); (5) Gonzalez et al. (1997a); (6) Rao et al. (2012); (7) Rao & Giridhar (2014); (8) Gorlova et al. (2012); (9) Maas et al. (2007); (10) Gonzalez et al. (1997b); (11) Gezer et al. (2015); (12) Maas et al. (2005); (13) Van Winckel (1997); (14) De Smedt et al. (2016); (15) Van Winckel (1995); (16) Waelkens et al. (1996); (17) Hrivnak et al. (2008); (18) Waelkens et al. (1991); (19) Kipper (2013); (20) Maas et al. (2003); (21) Van Winckel et al. (2012); (22) Giridhar et al. (1994); (23) Giridhar et al. (2000); (24) Maas et al. (2002); (25) Gonzalez & Wallerstein (1996).
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