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Table 6.
Upper limits of the Class I sources with no HI emission lines.
| ID | Lbol | SpT | AV | Lacc | SpTL |  |
|---|---|---|---|---|---|---|
| [L⊙] | [mag] | [L⊙] | ||||
| 147 | 0.08 | M5.5 | 30.0 | < 0.0025 | M9 | 33.0 |
| 161 | 0.06 | – | 20.0 | < 0.0009 | – | – |
| 183 | 1.20 | – | 20.0 | < 0.0094 | – | – |
| 190 (*) | 0.15 | M0.5 | 11.5 | < 0.0002 | – | – |
| 196 | 0.20 | M7.5 | 16.0 | < 0.0019 | M7.5 | 16.5 |
| 218 | 1.28 | – | 40.0 | < 0.0121 | – | – |
| 237 (*) | 0.06 | M4.5 | 5.0 | < 0.0001 | M2 | 5.86 |
Notes.
(*)
Sources whose bolometric luminosity was estimated as a lower limit because we have no photometry over the peak, see Fig. F.2.
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