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Table 4
Far-side IRDC candidates.
| Hi-GAL | Extinction1 | ||||
| ℓ | b | column | column | Temperature | |
| Source name | (°) | (°) | (×1022cm-2) | (×1022cm-2) | (K) |
|
|
|||||
| G030.60+0.18 | 30.602 | +0.177 | 6.2 | 1.1 | 22 |
| G030.34-0.11 | 30.345 | –0.114 | 1.7 | 0.15 | 19 |
| G030.01-0.272 | 30.006 | –0.270 | 3.1 | 0.5 | 21 |
| G029.31-0.05 | 29.312 | –0.051 | 1.0 | 0.06 | 13 |
| G029.28-0.33 | 29.284 | –0.331 | 1.6 | 0.02 | 20 |
Notes.
(1)
Not knowing the distances to all these sources, we use the Peretto & Fuller (2009) extinction column density estimation method, which basically assumes the cloud is on the near-side of the Galaxy.
(2)
This is the source that is discussed in the text in Sect. 5.
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