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Table A.6
Equivalent widths, HFS corrections (labeled “HFS” on top of the respective columns), and Mn abundance for the Mn i λ5407, λ5420, λ5432, and λ5516 lines observed for the stars of the Carina dSph galaxy.
| λ5407 | λ5420 | λ5432 | λ5516 | |||||||||||||
| Star | EW | HFS | [Mn/H] | [Mn/Fe] | EW | HFS | [Mn/H] | [Mn/Fe] | EW | HFS | [Mn/H] | [Mn/Fe] | EW | HFS | [Mn/H] | [Mn/Fe] |
|
|
||||||||||||||||
| MKV_0458 | 59.0 | −0.12 | −2.17 | −0.57 | ||||||||||||
| ± 4.1 | ± 0.09 | |||||||||||||||
| MKV_04841 | 53.3 | −0.11 | −1.70 | −0.17 | 79.1 | −0.22 | −1.77 | −0.24 | 141.4 | −0.35 | −1.86 | −0.33 | 30.5 | −0.04 | −1.83 | −0.30 |
| ± 4.5 | ± 0.05 | ± 2.9 | ± 0.03 | ± 5.9 | ± 0.05 | ± 9.3 | ± 0.16 | |||||||||
| MKV_0514 | 22.0 | −0.01 | −2.84 | −0.52 | ||||||||||||
| ± 2.3 | ± 0.07 | |||||||||||||||
| MKV_05241 | 38.9 | −0.07 | −1.68 | 0.07 | 37.5 | −0.06 | −1.98 | −0.23 | 86.3 | −0.11 | −2.05 | −0.30 | ||||
| ± 1.8 | ± 0.03 | ± 3.5 | ± 0.05 | ± 4.5 | ± 0.05 | |||||||||||
| MKV_0596 | 21.0 | −0.05 | −1.76 | −0.22 | 31.0 | −0.09 | −1.86 | −0.32 | 53.0 | −0.12 | −1.90 | −0.36 | ||||
| ± 2.6 | ± 0.08 | ± 3.1 | ± 0.08 | ± 3.5 | ± 0.07 | |||||||||||
| MKV_06121 | 57.2 | −0.16 | −1.48 | −0.18 | 65.6 | −0.19 | −1.68 | −0.38 | 134.5 | −0.45 | −1.45 | −0.15 | 32.4 | −0.06 | −1.61 | −0.31 |
| ± 3.8 | ± 0.04 | ± 4.3 | ± 0.04 | ± 5.2 | ± 0.05 | ± 4.4 | ± 0.07 | |||||||||
| MKV_0640 | 33.0 | −0.08 | −1.88 | −0.15 | 26.0 | −0.06 | −2.28 | −0.55 | 65.0 | −0.13 | −2.34 | −0.61 | ||||
| ± 2.9 | ± 0.08 | ± 3.2 | ± 0.09 | ± 4.5 | ± 0.08 | |||||||||||
| MKV_0677 | 30.0 | −0.08 | −2.12 | −0.37 | 34.0 | −0.09 | −2.34 | −0.59 | 90.0 | −0.26 | −2.44 | −0.69 | ||||
| ± 3.1 | ± 0.08 | ± 2.9 | ± 0.08 | ± 4.6 | ± 0.07 | |||||||||||
| MKV_0698 | 91.0 | −0.35 | −1.75 | −0.27 | 115.0 | −0.58 | −1.88 | −0.40 | 62.0 | −0.15 | −1.81 | −0.33 | ||||
| ± 2.8 | ± 0.05 | ± 3.3 | ± 0.05 | ± 2.1 | ± 0.05 | |||||||||||
| MKV_07051 | 74.5 | −0.24 | −1.32 | 0.03 | 72.5 | −0.23 | −1.63 | −0.28 | 128.3 | −0.42 | −1.51 | −0.16 | 38.0 | −0.07 | −1.53 | −0.18 |
| ± 3.9 | ± 0.04 | ± 10.6 | ± 0.09 | ± 6.2 | ± 0.06 | ± 5.9 | ± 0.08 | |||||||||
| MKV_0729 | 53.0 | −0.13 | −1.47 | −0.08 | 27.0 | −0.05 | −1.66 | −0.27 | ||||||||
| ± 5.6 | ± 0.11 | ± 3.4 | ± 0.11 | |||||||||||||
| MKV_0733 | 48.0 | −0.13 | −1.59 | 0.05 | ||||||||||||
| ± 5.4 | ± 0.10 | |||||||||||||||
| MKV_0740 | 83.0 | −0.26 | −1.45 | −0.25 | ||||||||||||
| ± 7.7 | ± 0.13 | |||||||||||||||
| MKV_07691 | 74.8 | −0.21 | −1.47 | 0.21 | 76.3 | −0.11 | −1.86 | −0.18 | 34.8 | −0.06 | −1.44 | 0.24 | ||||
| ± 6.7 | ± 0.06 | ± 5.0 | ± 0.05 | ± 5.9 | ± 0.12 | |||||||||||
| MKV_0780 | 65.0 | −0.08 | −2.03 | −0.25 | ||||||||||||
| ± 6.1 | ± 0.10 | |||||||||||||||
| MKV_0825 | 62.0 | −0.24 | −1.70 | −0.27 | 123.0 | −0.55 | −2.01 | −0.58 | ||||||||
| ± 4.8 | ± 0.08 | ± 5.5 | ± 0.09 | |||||||||||||
| MKV_0840 | 53.0 | −0.21 | −2.01 | −0.83 | 89.0 | −0.36 | −2.24 | −1.06 | ||||||||
| ± 4.8 | ± 0.10 | ± 3.0 | ± 0.10 | |||||||||||||
| MKV_0880 | 50.0 | −0.13 | −2.04 | −0.46 | 67.0 | −0.23 | −2.17 | −0.59 | 116.0 | −0.37 | −2.48 | −0.90 | 32.0 | −0.06 | −2.11 | −0.53 |
| ± 3.9 | ± 0.06 | ± 3.0 | ± 0.06 | ± 4.9 | ± 0.06 | ± 2.7 | ± 0.07 | |||||||||
| MKV_0900 | 36.0 | −0.10 | −2.21 | −0.49 | 111.0 | −0.43 | −2.53 | −0.81 | 29.0 | −0.06 | −2.16 | −0.44 | ||||
| ± 2.8 | ± 0.06 | ± 4.1 | ± 0.06 | ± 3.6 | ± 0.08 | |||||||||||
| MKV_0902 | 54.0 | −0.08 | −2.61 | −0.62 | ||||||||||||
| ± 6.7 | ± 0.08 | |||||||||||||||
| MKV_1007 | 58.0 | −0.28 | −1.76 | −0.37 | 53.0 | −0.24 | −2.10 | −0.71 | 102.0 | −0.55 | −2.23 | −0.84 | 37.0 | −0.12 | −1.84 | −0.45 |
| ± 4.3 | ± 0.09 | ± 4.0 | ± 0.09 | ± 2.8 | ± 0.09 | ± 3.1 | ± 0.09 | |||||||||
| MKV_1009 | 71.0 | −0.13 | −2.11 | −0.36 | ||||||||||||
| ± 7.9 | ± 0.12 | |||||||||||||||
| MKV_10131 | 32.9 | −0.06 | −1.66 | −0.36 | 89.3 | −0.29 | −1.40 | −0.10 | 92.0 | −0.17 | −1.79 | −0.49 | ||||
| ± 4.6 | ± 0.07 | ± 4.2 | ± 0.04 | ± 4.9 | ± 0.05 | |||||||||||
Notes.
(1)
From FLAMES-UVES spectra (Venn et al. 2012).
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