Table 3.
Correlation between the 12CO(J = 1 − 0) luminosity surface density and SFR surface density.
| Galaxy | N | r | pr | ρ | pρ | α1 | C1 |
|---|---|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
| NGC628 | 97 | 0.49 | 0.00 | 0.33 | 0.00 | 1.21 ± 0.13 | 2.25 ± 0.34 |
| NGC1808 | 20 | 0.89 | 0.00 | 0.87 | 0.00 | 1.56 ± 0.22 | 2.14 ± 0.38 |
| NGC4568 | 48 | 0.82 | 0.00 | 0.84 | 0.00 | 0.75 ± 0.07 | 1.15 ± 0.15 |
| Circinus galaxy | 11 | 0.85 | 0.00 | 0.91 | 0.00 | 1.80 ± 0.20 | 2.55 ± 0.33 |
| NGC3627 arm | 35 | 0.80 | 0.00 | 0.81 | 0.00 | 0.83 ± 0.07 | 1.10 ± 0.13 |
| NGC3627 bar | 9 | −0.58 | 0.10 | −0.68 | 0.04 | −0.28 ± 0.14 | −1.44 ± 0.31 |
| NGC1365 bar | 26 | 0.73 | 0.00 | 0.84 | 0.00 | 2.91 ± 0.39 | 3.19 ± 0.51 |
| NGC1365 arm | 11 | 0.21 | 0.54 | 0.36 | 0.28 | 6.10 ± 5.68 | 12.37 ± 12.52 |
Notes. This table shows (1) name, (2) number of data points for fitting, (3) the Pearson correlation coefficient, (4) the probability of the Pearson correlation, (5) the Spearman rank correlation, (6) the probability of the Spearman rank correlation, (7) the fitting power law index in Eq. (6), (8) the fitting constant in Eq. (6).
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