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Table 3
Class I accretion properties.
| Name | FBrγ a | FPfγ a | FBrα a | APfγ b | FBrα c | Log10Lacc d | |
|---|---|---|---|---|---|---|---|
| (10−17 W/m2) | (10−17 W/m2) | (10−17 W/m2) | (mag) | (mag) | (L⊙) | ||
| 1 | SSTc2d j162621.3-242304 | 5.3 ± 0.5 | <7 | 26.3 ± 4.0 | <2.1 | 2.1 ± 0.6 | 0.80 ± 0.59 |
| 2 | SSTc2d j162702.3-243727 | 18.5 ± 0.5 | 37.6 ± 1.8 | 133.9 ± 2.8 | 2.8 ± 0.4 | 2.6 ± 0.4 | 1.89 ± 0.39 |
| 3 | SSTc2d j162709.4-243718 | 20.1 ± 0.6 | 68 ± 11 | 209 ± 30 | 3.6 ± 0.5 | 3.0 ± 0.5 | 2.35 ± 0.51 |
| 4 | SSTc2d j162721.7-242953 | <1.0 | <2 | 11.1 ± 1.1 | – | – | − |
| 5 | SSTc2d j162726.9-244050 | 1.3 ± 0.2 | <3 | 15.0 ± 0.9 | <3.0 | 3.2 ± 0.5 | 1.01 ± 0.51 |
| 6 | SSTc2d j162727.9-243933 | 2.0 ± 0.2 | <5 | 16.54 ± 1.7 | <3.1 | 2.8 ± 0.5 | 0.86 ± 0.54 |
| 7 | SSTc2d j162730.1-242743 | 0.6 ± 0.16 | <3 | <8.2 | – | – | − |
| 8 | SSTc2d j163135.6-240129 | 1.0 ± 0.1 | 2.4 ± 0.4 | 12.9± 0.8 | 3.1 ± 0.6 | 3.32 ± 0.5 | 0.99 ± 0.50 |
| 9 | SSTc2d j163200.9-245642 | <0.7 | <3 | 9.8 ± 1.5 | – | – | − |
| 10 | IRAS 04016+2610 | <3 | <4 | 9.8 ± 1.6 | – | – | − |
| 11 | MHO 1 | 11.1 ± 0.6 | 6.1 ± 0.6 | 24.0 ± 1.0 | 0.9 ± 0.6 | 1.1 ± 0.4 | 0.16 ± 0.48 |
| 12 | MHO 2 | 9.0 ± 0.9 | <3 | 8.63 ± 0.9 | <0.2 | 0.1 ± 0.5 | −0.88 ± 0.59 |
| 13 | SSTtau 041430.5+280514 | 3.9 ± 0.6 | <2 | 6.8 ± 0.5 | <0.5 | 0.8 ± 0.5 | . −0.65 ± 0.58 |
| 14 | SSTtau 042107.9+270220 | 0.9 ± 0.06 | 0.7 ± 0.1 | 5.1 ± 0.06 | 1.4 ± 0.6 | 2.2 ± 0.4 | −0.11 ± 0.47 |
| 15 | SSTtau 042111.4+270109 | 1.8 ± 0.15 | 1.0 ± 0.1 | 2.8 ± 0.2 | 0.9 ± 0.5 | 0.67 ± 0.5 | −1.20 ± 0.56 |
| 16 | SSTtau 043232.0+225726 | 1.1 ± 0.13 | 0.9 ± 0.2 | 2.4 ± 0.3 | 1.4 ± 0.7 | 1.1 ± 0.5 | −1.05 ± 0.62 |
| 17 | SSTtau 043935.1+254144 | 1.4 ±0.07 | 3.4±0.3 | 13.5± 0.5 | 3.1±0.5 | 3.0± 0.4 | 0.79 ± 0.46 |
| 18 | IRAS04108+2803B | 0.3 ± 0.1 | 2.8 ± 0.1 | 9.6 ± 0.4 | 4.9 ± 0.5 | 4.3 ± 0.5 | 1.25 ± 0.48 |
| 19 | IRAS04158+2805 | 0.2 ± 0.06 | <0.4 | 1.0 ± 0.2 | <3 | 2.3 ± 0.8 | −0.96 ± 0.79 |
| 20 | IRAS04181+2654A | 0.8 ± 0.1 | 1.5 ± 0.3 | 5.3 ± 0.3 | 2.6 ± 0.7 | 2.44 ± 0.5 | 0.23 ± 0.54 |
| 21 | IRAS04239+2436 | 5.3 ± 0.06 | 11.7 ± 0.2 | 31.9 ± 0.4 | 2.9 ± 0.3 | 2.4 ± 0.4 | 0.94 ± 0.40 |
| 22 | IRAS04295+2251 | 0.4 ± 0.1 | <0.3 | 1.8 ± 0.2 | <1.4 | 2.0 ± 0.7 | −0.55 ± 0.66 |
| 23 | IRAS04361+2547 | 0.9 ± 0.06 | 1.0 ± 0.1 | 2.8 ± 0.08 | 1.9 ± 0.5 | 1.5 ± 0.4 | −0.78 ± 0.50 |
| 24 | IRAS04365+2535 | 1.3 ± 0.1 | 2.7 ± 0.3 | 13.1 ± 0.2 | 2.9 ± 0.5 | 3.02 ± 0.4 | 0.79 ± 0.45 |
Notes. (a) Observed fluxes: objects 1–17 are from this paper, objects 18–24 are from Beck. (b) Extinction at the Pfγ wavelength from the ratio Brγ/Pfγ.(c) Extinction at the Brα wavelength from the ratio Brα/Brγ. (d) Accretion luminosity computed from the Brα luminosity (eq.(2)).
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