Table 9.
Monte Carlo results for the proper motions and predicted positions 0.88 Ma ago for the 18 star sample.
| Name | Gaia DR3 ID | μα* | μδ | μα* | μδ | Δα | Δδ |
|---|---|---|---|---|---|---|---|
| (mas/a) | (mas/a) | (mas/a) | (mas/a) | (′) | (′) | ||
| Measured | Predicted | Predicted | |||||
| GLS 13 370 A | 431769183925254272 | 0.085 | −0.127 | 0.020 | 0.042 | −0.419 | −0.766 |
| GLS 13 362 | 431771863984836352 | −0.269 | 0.137 | −0.218 | 0.068 | 0.219 | −1.223 |
| GLS 13 376 | 431768943407111424 | 0.035 | −0.054 | 0.098 | −0.083 | −0.297 | −0.854 |
| GLS 13 368 | 431766950542328448 | −0.046 | −0.234 | −0.010 | −0.400 | −0.149 | −0.960 |
| GLS 22 355 | 431775334318395904 | −0.014 | 0.159 | −0.004 | 0.215 | −0.419 | −0.080 |
| GLS 13 365 | 431771623466692608 | −0.058 | −0.094 | −0.116 | −0.109 | −0.696 | −0.663 |
| GLS 22 356 | 431769287004467584 | 0.149 | 0.057 | 0.071 | 0.055 | −0.853 | −0.645 |
| 2MASS J00013526+6440324 | 431775330015871872 | −0.002 | 0.075 | 0.022 | 0.253 | −0.395 | −0.738 |
| 2MASS J00012544+6437439 | 431769252644723456 | −0.051 | 0.063 | −0.045 | 0.058 | −0.467 | −0.683 |
| GLS 13 370 D | 431769183925255680 | 0.094 | −0.071 | 0.041 | −0.030 | −0.875 | 0.127 |
| 2MASS J00012922+6437088 | 431769149565516288 | −0.022 | −0.016 | −0.021 | 0.018 | −0.411 | −0.676 |
| 2MASS J00013558+6433174 | 431768599809746688 | −0.092 | −0.412 | −0.066 | −0.394 | 0.930 | 0.996 |
| GLS 13 370 E | 431769183925258496 | 0.027 | 0.026 | 0.036 | 0.022 | −0.435 | −0.680 |
| 2MASS J00013231+6439510 | 431775231239186048 | 0.006 | 0.024 | −0.006 | 0.089 | −0.304 | 0.988 |
| GLS 13 370 C | 431769179623166976 | 0.073 | −0.023 | 0.007 | 0.029 | −0.353 | −0.591 |
| 2MASS J00014229+6436247 | 431768977766839168 | −0.004 | 0.105 | 0.059 | 0.034 | −0.197 | −1.651 |
| 2MASS J00015206+6437056 | 431769046486312320 | 0.001 | 0.011 | 0.084 | 0.017 | 0.484 | −0.710 |
| 2MASS J00014859+6433596 | 431768458064599040 | 0.203 | −0.121 | 0.131 | −0.191 | −0.577 | −0.757 |
Notes. Measured and predicted proper motions are relative to the mean value of sample 1 (μα * ,g, μδ, g) and the predicted positions are relative to the cluster center (αc, δc). The measured proper motions of GLS 13 370 A are those of GLS 13 370 B.
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