Table 2
Maximum and inner slope of the mean V3.6 μm, derived from the stellar contribution to the rotation curves, rescaled with respect to hR and the disk size in kpc.
| V3.6 μm parameters | 8.5 < log 10M∗/M⊙< 9 | 9 < log 10M∗/M⊙< 9.5 | 9.5 < log 10M∗/M⊙< 10 | 10 < log 10M∗/M⊙< 10.5 | 10.5 < log 10M∗/M⊙< 11 |
|
|
|||||
 (km s-1) |
31.2 (6.3) | 45.2 (10.6) | 72.7 (20.8) | 115.4 (26.2) | 160.4 (28.7) |
| dV3.6 μm(0) (km s-1 kpc-1) | 49.5 (19.1) | 79.2 (27.9) | 137.8 (56.2) | 241.7 (84.4) | 368.8 (85.1) |
dV3.6 μm(0) (km s-1 ) |
77.6 (41.7) | 135.7 (71.6) | 285.7 (179.9) | 651.4 (312.6) | 1134.1 (359.0) |
Notes. Parameters are given for the different stellar mass bins. In parentheses, we indicate the mean change in the parameters when using ⟨V3.6 μm⟩ ± σ instead of ⟨V3.6 μm⟩ (see error bars in Fig. 11).
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