Table C.3
Summary of star formation signposts for all the observed clumps.
| Clump | 24 μm Emission | MSX Emission | GF | 1.3 cm-Continuum | H2O Maser | Type |
|
|
||||||
| 08477−4359c1 | Y | Y? | ... | N | N | ... |
| 08589−4714c1 | Y | Y | ... | N | Y | ... |
| 12300−6119c1 | ... | Y | ... | N | N | ... |
| 13039−6331c1 | Y | Y | N | N | N | ... |
| 13560−6133c1 | Y | N | N | Y | Y | 2 |
| 13563−6109c1 | Y | Y | N | Y? | N | ... |
| 14166−6118c1 | Y | Y | N | Y | N | ... |
| 15072−5855c1 | Y | Y | Y | N | N | 2 |
| 15278−5620c1 | Y | Y | Y | Y | Y | 2 |
| 15278−5620c2 | Y | N | Y+ | N | N | 1 |
| 15470−5419c1 | N | N | Y | N | Y | 1 |
| 15470−5419c3 | Y | N | Y+ | N | Y | 1 |
| 15557−5215c1 | Y | Y | Y | N | Yc | 2 |
| 15557−5215c2 | Y | N | Y | N | Y | 1 |
| 15579−5303c1 | Y | Y | Y+ | Y | Y | 2 |
| 16061−5048c1 | Y | N | Y+ | Y | Y | 2 |
| 16061−5048c2 | Y | Y | Y+ | Y | Yc | 2 |
| 16061−5048c4 | N | N | N | Y | Y | 1 |
| 16093−5015c1 | Y | Y | Y+ | N | Nd | 1 |
| 16093−5128c1 | Y | Y | N | Y | N | 2 |
| 16093−5128c8 | N | N | Yb | N | N | 1 |
| 16164−4929c2 | Y | Y | N | Y | N | ... |
| 16254−4844c1 | Y | N | Y | Y | Nd | 1 |
| 16428−4109c1 | ... | Y | ... | Y | N | ... |
| 16428−4109c2 | ... | Y | ... | Y | N | ... |
| 16573−4214c2 | Y | N | Y | N | Ya | 1 |
| 17040−3959c1 | Y | N | N | N | N | 1 |
| 17195−3811c1 | Y | Y | Y | N | Ya | 2 |
| 17195−3811c2 | Y | N | Y | Y? | Ya | ... |
| 17195−3811c3 | Y | N | N | N | Ya | ... |
| 17355−3241c1 | Y | Y | N | N | N | 3 |
|
|
||||||
| 10088−5730c2 | ... | N | ... | N | N | ... |
| 13560−6133c2 | N | N | N | N | N | 1 |
| 14166−6118c2 | N | N | N | N | N | 1 |
| 14183−6050c3 | N | N | N | N | N | 1 |
| 15038−5828c1 | N | N | N | N | N | 1 |
| 15454−5335c2 | N | N | N | ... | N | ... |
| 15470−5419c4 | N | N | N | N | N | 1 |
| 15557−5215c3 | N | N | N | ... | N | 1 |
| 15579−5303c3 | N | N | N | ... | N | 1 |
| 16093−5128c2 | N | N | N | N | N | 1 |
| 16164−4929c3 | N | N | N | N | N | 1 |
| 16164−4929c6 | N | N | N | ... | N | ... |
| 16164−4837c2 | ... | N | N | ... | N | ... |
| 16435−4515c3 | N | N | N | Y? | N | ... |
| 16482−4443c2 | N | N | N | ... | N | 1 |
Notes.The clumps above the horizontal line are those classified as star-forming, while the clump below it are those classified as quiescent. For the “green fuzzies”, the notation Y+ indicates multiple “green fuzzies” associated with the clump. In the last column we show the Type of the source (see text).
These sources have poor uv-coverage, thus a firm assignment to a clump in the region was not possible.
Visual inspection of the Mid-IR images showed that this GF could be generated by the Spitzer PSF. However, we still consider the clump as star forming to be conservative, and because of the presence of a strong 24 μm source within the 3σ contour of the 1.2 mm continuum emission, at the location of the GF.
Source detected in our work, but not in that of Sánchez-Monge et al. (2013a).
Source detected in the work of Sánchez-Monge et al. (2013a), but not in our work.
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