Table 4
Emission detected toward the seven observed sources.
| Source name | Continuum | 12CO | N2 D+ | C18O | SiO | DCN | CH3OH | Outflow | |
|---|---|---|---|---|---|---|---|---|---|
| 7m | 12m | ||||||||
| AzTEC-lup1-2 | No | No | TP,7m(*) | TP | TP,7m(*) | No | TP | No | No |
| AzTEC-lup3-5 | No | No | TP,7m(*) | No | TP,7m(*) | No | No | No | No |
| IRAS 15398-3359 | Point-like | Point-like | TP,7m,12m | TP,7m | TP,7m,12m | TP,7m | TP,7m | TP | Yes |
| IRAS 16059-3857 | Point-like | Resolved | TP,7m,12m | TP | TP,7m | No | TP | No | Yes |
| J160115-41523 | Point-like | Resolved | TP,7m(*),12m | No | TP | No | No | No | Yes |
| Merin 28 | Point-like | Resolved | TP,7m | No | TP | No | No | No | Yes(**) |
| Sz 102 | Point like | Resolved | TP,7m | No | TP,7m(*) | No | No | No | Yes(**) |
Notes. Continuum emission, detected toward five sources, is identified as point-like in the dedicated 7m array observations(Band 6), while four of them are resolved in observations of 12m in Band 7 from the ALMA archive. (*) Only cloud emission is detected (no compact emission). In the last column we indicate in which sources we have detected 12CO(2–1) outflows associated. (**)Only signs of the presence of outflows are detected.
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