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Table 2
Derived star formation rates toward the four LABs.
| Source | SFR(LFIR) | SFR(L1.4 GHz) | log LLyαa | SFR(Lyα) |
| [M⊙/yr] | [M⊙/yr] | [erg s-1] | [M⊙/yr] | |
|
|
||||
| B1 | <480 | <1090 | 43.9 | 79 |
| B5 | <430 | 1090±340 | 43.8 | 63 |
| B6 | 1700±320 | 1430±360 | 43.8 | 63 |
| B7 | 1460±390 | 1650±340 | 43.5 | 32 |
Notes.
(a)
The Lyα luminosities are adopted from Colbert et al. (2006).
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