Table 6
Calculated luminosity values for the three protostellar cores in SDC335, assuming the ZAMS properties associated with each source in Paper I.
| L* |  |
Lacc (min) | Lacc (max) | Ltot,ZAMS (min) | Ltot,ZAMS (max) | Ltot,ZAMS∕Lbol factor | |
|---|---|---|---|---|---|---|---|
| Source | [L⊙] | [L⊙] | [L⊙] | [L⊙] | [L⊙] | ||
| MM1a | 5.5 × 103 | 1.3 × 104 | 1.3 × 104 | 7.6 × 104 | 1.9 × 104 | 8.1 × 104 | 1.4–6.2 |
| MM1b | 4.1 × 103 | 5.1 × 103 | 9.9 × 104 | 2.1 × 104 | 1.4 × 104 | 2.6 × 104 | 2.8–5.0 |
| MM2 | 4.4 × 103 | 9.9 × 103 | 1.7 × 102 | − | 4.5 × 103 | − | 0.5 |
Notes. This is a revised and expanded version of Table 6 in Paper I. For each source, we find a minimum and maximum Lacc and this Ltot,ZAMS based upon the range of Ṁacc between the red and blue outflow lobes from Table 5. (†)Lbol as derived in Paper I, the division of Lbol for the MM1 core is described within Sect. 4.2 of this paper.
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