Open Access
Table 1
Distances of the molecular clouds.
| Name | VLSR | COcut (1) | Dcut | Nstars | DTRI | DGAL | DLit(5) |
|---|---|---|---|---|---|---|---|
| (km s−1) | (K km s−1) | (pc) | (pc) | (pc) | (pc) | ||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
| G026.9 − 03.5 | 16.3 | 2.5 | 1000 | 263 |  |
 |
 |
| G027.8 − 02.1 | 18.0 | 4.2 | 1000 | 1876 |  |
 |
 |
| G028.6 − 02.9 | 18.5 | 0.9 | 1500 | 77 |  |
 |
 |
| G032.9 − 01.8 | 22.4 | 0.8 | 4000 | 113 |  |
 |
 |
| G034.2 − 01.7 | 6.6 | 2.0 | 1500 | 244 |  |
 |
 |
| G037.0 + 04.6 | 22.8 | 1.2 | 2000 | 164 |  |
 |
 |
| G038.1 − 01.2 | 7.7 | 2.0 | 2000 | 301 |  |
 |
|
| G038.4 − 03.3 | 7.5 | 1.5 | 2000 | 302 |  |
 |
|
| G039.4 − 02.7 | 15.0 | 2.5 | 1500 | 302 |  |
 |
 |
| G041.5 + 02.3 | 17.6 | 4.9 | 1500 | 1707 |  |
 |
 |
| G041.5 − 01.8 | 16.8 | 1.2 | 1500 | 304 |  |
 |
 |
| G041.9 + 02.2 | 5.4 | 1.5 | 800 | 1567 |  |
 |
 |
| G042.1 − 02.1 | 23.4 | 1.2 | 2000 | 335 |  |
 |
|
| G042.9 + 04.4 | 22.7 | 3.0 | 3500 | 49 |  |
 |
 |
| G043.3 + 03.1 | 10.2 | 2.5 | 1500 | 485 |  |
 |
 |
| G043.4 − 04.2 | 26.1 | 1.2 | 2000 | 102 |  |
 |
 |
| G044.5 + 02.7 | 14.6 | 2.0 | 1500 | 350 |  |
 |
 |
| G044.7 − 04.2 | 22.8 | 0.9 | 2000 | 104 |  |
 |
|
| G044.7 + 04.0 | 20.0 | 3.0 | 1500 | 1643 |  |
 |
 |
| G045.1 − 03.4 | 20.7 | 1.2 | 2000 | 196 |  |
 |
 |
| G045.4 − 04.2 | 18.8 | 2.5 | 1500 | 851 |  |
 |
 |
| G045.5 − 03.3 | 20.2 | 2.0 | 1500 | 133 |  |
 |
 |
| G046.9 − 04.8 | 15.7 | 0.9 | 1500 | 99 |  |
 |
 |
| G046.9 + 01.7 | 6.8 | 2.8 | 1000 | 298 |  |
 |
|
| G047.3 − 03.1 | 18.7 | 2.0 | 2000 | 177 |  |
 |
 |
| G047.3 − 03.0 | 24.4 | 1.5 | 2000 | 164 |  |
 |
|
| G049.4 − 04.6 | 18.7 | 0.9 | 2000 | 81 |  |
 |
 |
Notes. (1)The lower threshold of the CO emission for on-cloud stars. (2)The number of the on-cloud stars used to calculate the distance. (3)The estimated distances based on the TRILEGAL model. (4)The estimated distances based on the GALAXIA model. (5)The distances of Yan et al. (2021).
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