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Table 8.
Relation of different components of millimeter emission with SFR and H2.
| NGC 2146 | X | Y | a | rP | Y | a | rP |
|---|---|---|---|---|---|---|---|
| ΣLmm | ΣSFR | 1.5 ± 0.1 | 0.99 ± 0.01 | ΣH2 | 1.3 ± 0.1 | 0.97 ± 0.02 | |
| 1.15 mm | ΣLdust | ΣSFR | 1.6 ± 0.1 | 0.99 ± 0.01 | ΣH2 | 1.4 ± 0.2 | 0.97 ± 0.02 |
| ΣLRC | ΣSFR | 1.1 ± 0.1 | 0.97 ± 0.02 | ΣH2 | 0.9 ± 0.1 | 0.96 ± 0.03 | |
| ΣLmm | ΣSFR | 1.3 ± 0.1 | 0.99 ± 0.01 | ΣH2 | 1.1 ± 0.1 | 0.97 ± 0.02 | |
| 2 mm | ΣLdust | ΣSFR | 1.6 ± 0.1 | 0.98 ± 0.01 | ΣH2 | 1.4 ± 0.2 | 0.97 ± 0.02 |
| ΣLRC | ΣSFR | 1.1 ± 0.1 | 0.98 ± 0.02 | ΣH2 | 0.9 ± 0.1 | 0.96 ± 0.02 | |
| NGC 2976 | X | Y | a | rP | Y | a | rP |
| ΣLmm | ΣSFR | 2.5 ± 0.8 | 0.89 ± 0.04 | ΣH2 | 2.5 ± 1.0 | 0.78 ± 0.08 | |
| 1.15 mm | ΣLdust | ΣSFR | 2.9 ± 0.7 | 0.92 ± 0.03 | ΣH2 | 2.7 ± 0.9 | 0.87 ± 0.05 |
| ΣLRC | ΣSFR | 0.9 ± 0.1 | 0.78 ± 0.08 | ΣH2 | 0.9 ± 0.2 | 0.57 ± 0.13 | |
| ΣLmm | ΣSFR | 2.3 ± 0.5 | 0.86 ± 0.05 | ΣH2 | 2.3 ± 0.7 | 0.78 ± 0.08 | |
| 2 mm | ΣLdust | ΣSFR | 2.9 ± 0.7 | 0.91 ± 0.03 | ΣH2 | 2.8 ± 0.8 | 0.87 ± 0.05 |
| ΣLRC | ΣSFR | 1.0 ± 0.1 | 0.79 ± 0.08 | ΣH2 | 0.9±0.2 | 0.57 ± 0.13 | |
Notes. Parameters of the linear fits in logarithmic scales (log Y = alog X + b) in Fig. 11 obtained using the OLS-bisector method (Akritas & Bershady 1996) with rP the Pearson correlation coefficient.
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