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Table 7
Dust-attenuation corrections of the Hα emission using the formula from Kennicutt & Evans (2012) for the different objects observed with the IRAM 30 m.
| Source | 3C 285 | 3C 285/09.6 | NGC 541 | MO |
|
|
||||
|
25 | 2.8 | 0.13 | 6.6 |
| L24 μm(1042 erg s-1) | 110 | 3.8 | 0.74 | 0.66 |
|
245 | 10.4 | 1.61 | 7.92 |
|
|
||||
| SFR(M⊙ yr-1) | 14.53 | 0.62 | 0.095 | 0.47 |
| tdep(Gyr) | 0.71 | < 1.0 | 1.79 | 0.02 |
Notes. The SFR is calculated with the conversion formula (Kennicutt & Evans 2012).
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