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Table 6
Driving source candidates.
| Ser-emb- | α 2000 | δ 2000 | YSO | L bol | T bol | M disk |
| (h) | (deg) | (L⊙) | (K) | (M⊙) | ||
|
|
||||||
| 1 (MMS3) | 18 29 09.09 | 00 31 30.9 | 0 | 4.1 | 39 | 0.28 |
| 11 E | 18 29 06.75 | 00 30 34.4 | I | – | – | – |
| 11 W | 18 29 06.61 | 00 30 34.0 | I | 4.8 | 77 | 0.15 |
| 17 | 18 29 06.20 | 00 30 43.1 | I | 3.8 | 120 | 0.15 |
Notes.Values of Lbol and Tbol and estimates of disk masses, as well as positions from CARMA 230 GHz observations, are all from Enoch et al. (2009, 2011).
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