Table 2.
Star formation rates for the stripped material and total star formation rates over the entire galaxy.
| Bandpass | SFR in tails [M⊙ yr−1] |
Total SFR [M⊙ yr−1] |
|||
|---|---|---|---|---|---|
| NGC 3312 | NGC 3314a | NGC 3312 | NGC 3314a | LEDA 753342 | |
| FUV | 0.62 ± 0.24 | 0.53 ± 0.05 | 1.45 ± 0.35 | 1.33 ± 0.08 | 0.152 ± 0.010 |
| NUV | 0.72 ± 0.52 | 0.89 ± 0.11 | 2.60 ± 0.82 | 2.29 ± 0.16 | 0.245 ± 0.019 |
| Hα | 0.77 ± 0.81 | 0.38 ± 0.08 | 3.99 ± 1.00 | 1.70 ± 0.11 | 0.145 ± 0.012 |
| WISE 12 μm | – | – | 4.03 ± 1.40 | 3.85 ± 1.33 | 0.054 ± 0.021 |
Notes. See Fig. 6 for regions and text for explanation. Disk SFRs can be estimated from the total, minus stripped. These estimates do not account for intrinsic dust extinction within the galaxy and as such present lower limits to the actual star formation rate (and thus apparent trends with bandpass largely reflect the unknown effect of internal dust obscuration).
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