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Table 3.
Derived SFR properties.
| Galaxy | SFR20 | SFR20 | SFRW3PAH(a) |
|---|---|---|---|
| (> 5 M⊙ yr−1) | (> 0.1 M⊙ yr−1) | (M⊙ yr−1) | |
| NGC 2397 | 0.4 | 2.0 | 1.4 |
| NGC 2442 | 2.8 | 13.4 | 1.4 |
| ESO 059-G012 | 0.001 | 0.008 | 0.03 |
| NGC 2434 | 0.056 | 0.26 | ... |
| ESO 263-G033 | 0.01 | 0.06 | 0.003 |
| NGC 3256 | 20.6 | 98.15 | 50 |
| PGC 087403 | 0.1 | 0.02 | ... |
| LEDA 087403 | 0.02 | 0.10 | ... |
| LEDA 3097821 | 0.01 | 0.08 | ... |
| NGC 3256B | 1.6 | 7.62 | 2.1 |
| NGC 3261 | 2.81 | 13.40 | 2.2 |
| NGC 3256C | 0.99 | 4.74 | 1.6 |
| NGC 3263 | 6.41 | 30.5 | 7.9 |
| ESO 263-G044 | 0.09 | 0.43 | 0.03 |
| NGC 3256A | 0.008 | 0.04 | 0.01 |
| LEDA 533801 | 0.04 | 0.19 | ... |
| ESO 263-G046 | 0.03 | 0.14 | 0.03 |
| NGC 6215 | 2.8 | 13.5 | 3.2 |
| NGC 6221 | 3.4 | 16.3 | 7.7 |
Notes. References: SFR20 (Condon et al. 2002),
(a)
SFRW3PAH/0.67 to convert from Kroupa IMF to Salpeter IMF (Cluver et al. 2014).
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