Table A.1
Distances to YSOs based on the CO emission and the Gaia catalog (Bailer-Jones et al. 2021)
| Nr | IRAC Designationa ‘SSTSMOGA’ | RA (deg) | DEC (deg) | Separationb (arc sec) | DkinC(pc) | DGaiad (pc) | ||
|---|---|---|---|---|---|---|---|---|
| 50th | 14th | 86th | ||||||
| 1 | G104.6313+02.6211 | 334.176540 | 59.876274 | 0.60 | 2197 | 224 | 218 | 231 |
| 2 | G104.6829+02.6173 | 334.266213 | 59.901773 | 0.12 | 2197 | 1481 | 1227 | 1968 |
| 3 | G104.7023+02.8142 | 334.079104 | 60.076155 | 0.11 | 5628 | 6245 | 4413 | 9334 |
| 4 | G104.7061+02.7861 | 334.116800 | 60.054850 | 0.35 | 5628 | 8687 | 4425 | 10873 |
| 5 | G104.7062+02.7895 | 334.113200 | 60.057750 | 0.15 | 5628 | 1179 | 1157 | 1200 |
| 6 | G104.7153+02.7979 | 334.118870 | 60.069817 | 0.11 | 5628 | 9531 | 5675 | 15687 |
| 7 | G104.7241+02.8075 | 334.122770 | 60.082638 | 0.09 | 5628 | 7498 | 4365 | 9265 |
| 8 | G104.7418+02.5949 | 334.388550 | 59.915745 | 0.07 | 2215 | 5354 | 4070 | 6247 |
| 9 | G104.7538+02.8964 | 334.072570 | 60.172980 | 0.17 | 2208 | 506 | 454 | 577 |
| 10 | G104.8429+02.6522 | 334.493160 | 60.019398 | 1.05 | 2230 | 6691 | 4698 | 9651 |
| 11 | G104.9084+02.7625 | 334.480220 | 60.147484 | 0.02 | 2230 | 3839 | 3109 | 4469 |
| 12 | G104.9180+02.7798 | 334.477020 | 60.167213 | 0.18 | 2223 | 1673 | 1440 | 2567 |
Notes. (a) Sources with the differences in the distances calculated using CO and Gaia exceeding the Gaia uncertainties are in bold. (b)A separation between the YSO and the closest Gaia target from the Bailer-Jones et al. (2021) catalog. (c)A kinematic distance from the CO emission (Section 3.1). (d)The three quantiles of a distance distribution from Bailer-Jones et al. (2021): the median (the 50th percentile), the 14th, and 86th percentiles.
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