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Table 3
Mass flux estimations for jets and outflows in NGC 1333.
| Source | Tbol (a) | Lbol (a) | tdyn (b) |  |
ṀCO |  |
Ṁ[O I](c) | Ṁ[O I]−shock(c) |
|---|---|---|---|---|---|---|---|---|
| (K) | L⊙ | (103 yr) | (10−6 M⊙∕yr) | |||||
| SVS13A | 250 | 59 | 8.0 | 4.8 | 42.3 | 0.23 | 0.19 | 3.81 |
| SVS13C | 36 | 4.9 | 11.2 | 13.9 | 37.9 | 0.90 | 0.18 | 3.34 |
| IRAS 2A W-E | 57 | 76 | 7.1 | 0.65 | 2.71 | 0.03 | 0.01 | 0.12 |
| IRAS 2A S-N | 57 | 76 | 3.5 | 7.4 | 89.2 | 0.51 | 0.08 | 0.76 |
| IRAS 4A | 43 | 5.8 | 1.3 | 5.3 | 23.6 | 0.51 | 0.14 | 0.49 |
| SK14 | 59 | 0.2 | 2.4 | 2.0 | 10.1 | 0.05 | 0.09 | 0.53 |
| SK1 | 32 | 0.7 | 2.3 | 4.0 | 23.8 | 0.11 | 0.03 | 0.18 |
Notes. (a) Source bolometric temperatures and luminosities are from Plunkett et al. (2013). (b) Dynamical scale is the average from the two lobes, as reported in Table 2. (c) [OI] mass flux values are from Paper I and is reported here to enable comparisons.
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