Table 3.
Mean parameter values calculated for the different structure components using the CALIFA V500 data cubes (e.g., Sánchez et al. 2016a).
| C | bl | bar | disk | N | |
|---|---|---|---|---|---|
| σ (all) | 210 ± 5 | 157 ± 9 | 132 ± 9 | − | 25 |
| σ (bulge) | 212 ± 7 | 147 ± 15 | 127 ± 12 | − | 11 |
| σ (no bulge) | 207 ± 7 | 165 ± 10 | 137 ± 14 | − | 14 |
| Age (m, all) | 8.8 ± 0.2 | 8.7 ± 0.2 | 8.3 ± 0.4 | 8.3 ± 0.1 | 25 |
| Age (m, bulge) | 9.0 ± 0.4 | 8.8 ± 0.2 | 8.7 ± 0.3 | 8.3 ± 0.2 | 11 |
| Age (m, no bulge) | 8.7 ± 0.2 | 8.7 ± 0.2 | 7.9 ± 0.6 | 8.2 ± 0.2 | 14 |
| Age (l, all) | 5.3 ± 0.5 | 5.4 ± 0.4 | 5.2 ± 0.4 | 4.1 ± 0.3 | 25 |
| Age (l, bulge) | 5.8 ± 0.7 | 5.7 ± 0.6 | 5.6 ± 0.6 | 4.5 ± 0.5 | 11 |
| Age (l, no bulge) | 4.9 ± 0.7 | 5.1 ± 0.5 | 4.8 ± 0.5 | 3.9 ± 0.3 | 14 |
| log10Z/Z⊙ (m, all) | −0.06 ± 0.02 | −0.02 ± 0.03 | −0.04 ± 0.03 | −0.12 ± 0.02 | 25 |
| log10 Z/Z⊙ (m, bulge) | −0.04 ± 0.03 | −0.03 ± 0.03 | 0.00 ± 0.03 | −0.09 ± 0.02 | 11 |
| log10 Z/Z⊙ (m, no bulge) | −0.01 ± 0.04 | −0.03 ± 0.04 | −0.06 ± 0.04 | −0.14 ± 0.04 | 14 |
| log10 Z/Z⊙ (l, all) | −0.10 ± 0.02 | −0.10 ± 0.02 | −0.09 ± 0.02 | −0.19 ± 0.02 | 25 |
| log10 Z/Z⊙ (l, bulge) | −0.08 ± 0.03 | −0.09 ± 0.03 | −0.06 ± 0.03 | −0.17 ± 0.02 | 11 |
| log10 Z/Z⊙ (l, no bulge) | −0.12 ± 0.03 | −0.10 ± 0.03 | −0.11 ± 0.04 | −0.20 ± 0.03 | 14 |
| g′−r′ (all) | 0.885 ± 0.013 | 0.824 ± 0.010 | 0.825 ± 0.010 | 0.769 ± 0.011 | 25 |
| g′ − r′ (bulge) | 0.887 ± 0.022 | 0.816 ± 0.012 | 0.815 ± 0.013 | 0.767 ± 0.016 | 11 |
| g′−r′ (no bulge) | 0.884 ± 0.017 | 0.830 ± 0.016 | 0.833 ± 0.014 | 0.772 ± 0.015 | 14 |
| r′−i′ (all) | 0.404 ± 0.017 | 0.419 ± 0.005 | 0.400 ± 0.017 | 0.395 ± 0.017 | 24 |
| r′−i′ (bulge) | 0.415 ± 0.006 | 0.410 ± 0.007 | 0.410 ± 0.007 | 0.409 ± 0.009 | 10 |
| r′−i′ (no bulge) | 0.395 ± 0.031 | 0.426 ± 0.007 | 0.390 ± 0.031 | 0.382 ± 0.030 | 14 |
Notes. The regions used are shown in Fig. 11, explained in Sect. 7.2. The galaxies with (bulge) and without (no bulge) a separately fitted bulge component are shown separately. The parameters are stellar velocity dispersion (σ) [km s−1], mass (“m”) and light (“l”) weighted stellar ages [Gyrs], and metallicity in respect to solar metallicity (log10Z/Z⊙). The (g′-r′) and (r′-i′) colors obtained from the SDSS mosaic images are also shown. The uncertainties are calculated from the sample standard deviation, divided by square-root of sample size. One of the galaxies did not have an i′-band image.
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