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Table D.4

The chemical abundances derived for NGC 6397 stars (69.D-0220(B)) with GALA using atmospheric parameters from spectral line profile fitting as starting values (Table C.2). The references for the line parameters used for the analysis can be found in Table E.1.

T170 T172 T179 T183
Teff [K] 11550 11100 10800 11300
log g [cm s–2] 3.80 3.75 3.40 3.30
vturb [km s–1] 0.7 0.2 0.3 0.0

ion [M/H] nlin [M/H] nlin [M/H] nlin [M/H] nlin
[Fe I/H] –0.24±0.06 10 +0.08±0.08 10 –0.18±0.07 9 +0.25±0.10 6
[Fe II/H] –0.22±0.12 37 +0.07±0.14 46 –0.17±0.09 50 +0.27±0.15 47

α elements

[Si II/H] –1.79±0.08 4 –1.67±0.06 5
[Ti II/H] +0.45±0.06 17

iron-peak elements

[Mn II/H] +0.36±0.03 2
T185 T186 T191 T193
Teff [K] 11050 11250 11150 11550
log g [cm s–2] 3.50 3.60 3.60 3.60
vturb [km s–1] 0.0 0.0 0.0 0.0

ion [M/H] nlin [M/H] nlin [M/H] nlin [M/H] nlin
[Fe I/H] –0.26±0.05 8 +0.09±0.09 12 –0.21±0.12 3 +0.25±0.10 13
[Fe II/H] –0.28±0.06 29 +0.10±0.13 79 –0.32±0.10 19 +0.27±0.11 96

α elements

[Ti II/H] +0.67±0.08 39 +1.28±0.09 19 +0.34±0.06 19

iron-peak elements

[Cr II/H] –0.45±0.04 3 +0.08±0.09 9 +0.04±0.01 2 –0.13±0.06 4
[Mn II/H] +1.10±0.15 10 +1.03±0.23 8 +1.18±0.10 11

other elements

[Y II/H] +1.71±0.03 3 +1.67±0.03 2

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