Table 7
Overview of the four s-process indices of the stars in Figs. 12 and 13.
| Object | [Fe/H] | C/O | [ls/Fe] | [hs/Fe] | [s/Fe] | [hs/ls] |
|
|
||||||
| IRAS 04296+3429a | –0.62 ± 0.20 | 1.66 ± 0.12 | 1.34 ± 0.07 | 1.45 ± 0.06 | –0.32 ± 0.14 | |
| IRAS 05341+0852a | –0.85 ± 0.20 | 1.4 ± 0.3 | 1.92 ± 0.08 | 2.30 ± 0.07 | 2.17 ± 0.05 | 0.38 ± 0.11 |
| IRAS 06530-0213b | –0.46 ± 0.20 | 2.8 ± 0.3 | 1.82 ± 0.09 | 2.11 ± 0.07 | 2.02 ± 0.05 | 0.29 ± 0.11 |
| IRAS 07134+1005a | –1.00 ± 0.20 | 1.0 ± 0.3 | 1.55 ± 0.17 | 1.36 ± 0.07 | 1.43 ± 0.07 | –0.19 ± 0.18 |
| IRAS 08143-4406b | –0.39 ± 0.20 | 1.3 ± 0.3 | 1.52 ± 0.15 | 1.49 ± 0.07 | 1.50 ± 0.07 | –0.03 ± 0.16 |
| IRAS 19500-1709a | –0.60 ± 0.20 | 1.1 ± 0.3 | 1.38 ± 0.11 | 0.90 ± 0.07 | 1.06 ± 0.06 | –0.48 ± 0.13 |
| IRAS 22223+4327a | –0.31 ± 0.20 | 1.2 ± 0.3 | 1.55 ± 0.10 | 1.25 ± 0.09 | 1.35 ± 0.07 | –0.30 ± 0.14 |
| IRAS 23304+6147a | –0.79 ± 0.20 | 2.9 ± 0.3 | 1.55 ± 0.10 | 1.50 ± 0.09 | 1.52 ± 0.07 | –0.05 ± 0.14 |
| J004441.04-732136.4c | –1.34 ± 0.17 | 1.9 ± 0.7 | 2.06 ± 0.10 | 2.58 ± 0.10 | 2.40 ± 0.10 | 0.52 ± 0.10 |
| J050632.10-714229.9d | –1.15 ± 0.17 | 1.5 ± 0.3 | 1.42 ± 0.07 | 1.07 ± 0.14 | 1.19 ± 0.09 | –0.35 ± 0.15 |
| J051213.81-693537.1e | –0.56 ± 0.15 | 1.3 ± 0.4 | 1.33 ± 0.08 | 1.74 ± 0.08 | 1.61 ± 0.06 | 0.41 ± 0.12 |
| J051848.86-700246.9e | –1.03 ± 0.14 | 1.3 ± 0.3 | 1.46 ± 0.10 | 2.12 ± 0.08 | 1.90 ± 0.07 | 0.66 ± 0.13 |
| J052043.86-692341.0d | –1.15 ± 0.17 | 1.6 ± 0.9 | 1.67 ± 0.12 | 1.85 ± 0.10 | 1.79 ± 0.08 | 0.19 ± 0.16 |
| J053250.69-713925.8d | –1.22 ± 0.11 | 2.5 ± 0.7 | 1.51 ± 0.16 | 1.94 ± 0.10 | 1.80 ± 0.08 | 0.43 ± 0.19 |
Notes.
Galactic object, from Van Winckel & Reyniers (2000). For C/O, we assume an uncertainty of 0.3 dex.
Galactic object, from Reyniers et al. (2004). For C/O, we assume an uncertainty of 0.3 dex.
SMC object, from De Smedt et al. (2012).
LMC object, from van Aarle et al. (2013).
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