Table 4.
Spatially resolved RC–SFR relation, the (ΣSFR)RC–(ΣSFR)hyb relation, at 1.2 kpc spatial resolution.
| Galaxy | a1 | b1 | σ1, 1200 | a2 | b2 | σ2, 1200 | FWHM1200 |
|---|---|---|---|---|---|---|---|
| (dex) | (dex) | (arcsec) | |||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
| NGC 3184 | 0.46 ± 0.02 | −1.49 ± 0.06 | 0.12 | 0.60 ± 0.02 | −0.98 ± 0.05 | 0.10 | 22.29 |
| NGC 4736 | 0.72 ± 0.02 | −0.74 ± 0.07 | 0.10 | 0.80 ± 0.03 | −0.21 ± 0.08 | 0.12 | 52.64 |
| NGC 5055 | 0.68 ± 0.02 | −0.53 ± 0.04 | 0.15 | 0.84 ± 0.02 | −0.13 ± 0.05 | 0.16 | 24.50 |
| NGC 5194 | 0.51 ± 0.02 | −0.69 ± 0.04 | 0.20 | 0.76 ± 0.02 | −0.08 ± 0.05 | 0.22 | 30.93 |
| Combineda | 0.59 ± 0.02 | −0.77 ± 0.05 | 0.31 | 0.79 ± 0.02 | −0.23 ± 0.04 | 0.25 | − |
| Young CREb | 0.93 ± 0.03 | −0.21 ± 0.06 | 0.21 | 0.91 ± 0.03 | −0.04 ± 0.06 | 0.21 | − |
Notes. Columns: (1) data plotted; (2,3) best-fitting parameters for Eq. (3) for ν1 ≈ 140 MHz; (4) standard deviations for ν1; (5,6) best-fitting parameters for Eq. (3) for ν2 = 1365 MHz; (7) standard deviations for ν2; (8) angular resolution given as FWHM of the map, which is equivalent to a projected spatial resolution of 1.2 kpc. (a)Relation for the plot of the combined data points from the galaxy sample as presented in Fig. 5; (b)relation for young CREs using only data points for which α > −0.65 as presented in Fig. 6.
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