Table 7:
Comparison between Fe I abundances from spectrum synthesis and 
analysis for observed stars in NGC 2506, NGC 6134, and IC 4651.
| Star |
[Fe/H]I |
rms |
n |
[Fe/H]I |
Phase |
| |
SS |
|
|
|
|
| NGC 2506 |
| 459 |
-0.42 |
0.264 |
30 |
-0.37 |
RGBtip |
| 438 |
-0.21 |
0.144 |
26 |
-0.18 |
clump |
| 443 |
-0.15 |
0.079 |
19 |
-0.21 |
clump |
| 456 |
-0.31 |
0.206 |
27 |
-0.21 |
RGB |
| NGC 6134 |
| 404 |
+0.12 |
0.145 |
22 |
+0.11 |
clump |
| 929 |
+0.20 |
0.224 |
23 |
+0.24 |
clump |
| 875 |
+0.10 |
0.253 |
29 |
+0.16 |
clump |
| 428 |
+0.19 |
0.049 |
11 |
+0.22 |
clump |
| 421 |
+0.09 |
0.148 |
16 |
+0.11 |
clump |
| 527 |
+0.09 |
0.218 |
21 |
+0.05 |
clump |
| IC 4651 |
| 27 |
+0.16 |
0.200 |
25 |
+0.10 |
clump |
| 76 |
+0.07 |
0.141 |
19 |
+0.10 |
clump |
| 72 |
+0.18 |
0.172 |
21 |
+0.13 |
RGB |
| 56 |
-0.68 |
0.238 |
24 |
-0.34 |
RGBtip |
| 146 |
+0.18 |
0.198 |
23 |
+0.10 |
clump |
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