Table 2
Sources from our protostar catalogue with a Gaia counterpart within 10′′.
| ID | RA | Dec | Distance | ID | RA | Dec | Distance | ID | RA | Dec | Distance |
|---|---|---|---|---|---|---|---|---|---|---|---|
| 1) | 51.27800 | 31.11428 | 299 ± 10 | 10) | 52.23893 | 31.23733 | 291 ± 10 | 19) | 55.41336 | 31.60310 | 300 ± 11 |
| 2) | 51.28956 | 30.77220 | 285 ± 65 | h2) | 52.26552 | 31.26772 | 240 ± 36 | 20) | 55.49376 | 31.81556 | 312 ± 25 |
| h1) | 51.41199 | 30.73479 | 237 ± 26 | 11) | 52.37169 | 31.30924 | 315 ± 24 | 21) | 55.72903 | 31.72932 | 330 ± 13 |
| 3) | 51.45769 | 31.17290 | 292 ± 11 | 12) | 52.47598 | 31.34729 | 296 ± 17 | 22) | 55.73202 | 31.97893 | 313 ± 10 |
| 4) | 51.61836 | 31.20151 | 292 ± 14 | 13) | 52.71848 | 30.90509 | 327 ± 66 | 23) | 56.11088 | 32.07526 | 330 ± 19 |
| 5) | 51.94876 | 30.20121 | 250 ± 29 | 14) | 52.82618 | 30.82677 | 302 ± 12 | 24) | 56.14806 | 32.15777 | 333 ± 89 |
| 6) | 52.15382 | 31.29370 | 374 ± 60 | 15) | 52.87012 | 30.51453 | 295.1 ± 8.6 | 25) | 56.31799 | 32.10562 | 308 ± 23 |
| 7) | 52.18035 | 31.29248 | 205 ± 36 | 16) | 53.14148 | 31.01549 | 307 ± 19 | 26) | 56.33484 | 32.10952 | 310 ± 20 |
| 8) | 52.21291 | 31.30397 | 296 ± 31 | 17) | 55.19518 | 32.53161 | 308 ± 13 | 27) | 56.45099 | 32.40305 | 311 ± 13 |
| 9) | 52.23529 | 31.30954 | 345 ± 40 | 18) | 55.28775 | 31.74389 | 326 ± 28 | 28) | 56.94595 | 33.06746 | 343 ± 76 |
Notes. We listed also h1 (L1448 C) and h2 (SVS13 in NGC1333) which host masers from which an astrometric distance was obtained (Hirota et al. 2008, 2011). For all the sources, the distance in parsec was derived from parallax according to Luri et al. (2018).
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