Table 5.
Median MassW [Z/H] measured for each environment in each galaxy.
| Target | Disk | Sp. arms | Bar | Ring | Center | All |
|---|---|---|---|---|---|---|
| NGC 0628 | –0.30±0.23 | –0.31±0.25 | – | – | –0.24±0.14 | –0.30±0.24 |
| NGC 1087 | –0.33±0.27 | – | –0.23±0.22 | – | – | –0.30±0.28 |
| NGC 1300 | –0.00±0.22 | –0.09±0.24 | –0.07±0.13 | –0.01±0.09 | –0.05±0.11 | –0.03±0.22 |
| NGC 1365 | –0.12±0.24 | –0.11±0.24 | –0.00±0.13 | 0.07±0.11 | 0.13±0.10 | –0.07±0.23 |
| NGC 1385 | –0.13±0.28 | –0.27±0.26 | – | – | – | –0.13±0.28 |
| NGC 1433 | 0.00±0.18 | – | –0.03±0.11 | –0.01±0.17 | 0.22±0.05 | –0.00±0.17 |
| NGC 1512 | –0.00±0.24 | –0.04±0.25 | –0.02±0.08 | –0.01±0.19 | 0.02±0.05 | –0.01±0.21 |
| NGC 1566 | –0.18±0.21 | –0.13±0.23 | –0.09±0.11 | – | – | –0.16±0.21 |
| NGC 1672 | –0.30±0.23 | –0.30±0.26 | –0.16±0.16 | 0.01±0.11 | 0.05±0.12 | –0.26±0.22 |
| NGC 2835 | –0.49±0.29 | –0.47±0.27 | –0.35±0.19 | – | – | –0.48±0.28 |
| NGC 3351 | –0.00±0.17 | – | –0.02±0.08 | 0.02±0.14 | 0.05±0.08 | 0.00±0.15 |
| NGC 3627 | –0.02±0.20 | –0.02±0.21 | 0.04±0.10 | – | 0.10±0.07 | –0.01±0.20 |
| NGC 4254 | –0.19±0.27 | –0.19±0.28 | – | – | –0.15±0.10 | –0.16±0.28 |
| NGC 4303 | –0.09±0.24 | –0.17±0.26 | 0.09±0.10 | – | 0.15±0.07 | –0.10±0.25 |
| NGC 4321 | –0.15±0.23 | –0.11±0.22 | –0.10±0.15 | 0.20±0.09 | 0.07±0.14 | –0.13±0.22 |
| NGC 4535 | –0.14±0.15 | –0.06±0.15 | –0.11±0.10 | – | –0.01±0.13 | –0.13±0.15 |
| NGC 5068 | –0.48±0.28 | – | –0.41±0.21 | – | – | –0.48±0.28 |
| NGC 7496 | –0.20±0.22 | – | –0.19±0.18 | – | – | –0.20±0.21 |
| IC 5332 | –0.56±0.23 | – | – | – | –0.40±0.20 | –0.54±0.23 |
| Offset to median | –0.01±0.24 | –0.01±0.25 | 0.03±0.14 | 0.00±0.17 | 0.10±0.16 | – |
| (all galaxies) | ||||||
Notes. The right-most column shows the median MassW [Z/H] across the full MUSE mosaic, considering all environments. Errors correspond to the standard deviation of the MassW [Z/H] distribution within each environment. The bottom row shows the median offset (in dex, for the full sample) of the MassW [Z/H] distribution within each environment of a given galaxy, with respect to the overall distribution (considering all environments) of the same galaxy.
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