Coordinates, proper motions, parallax, and radial velocity (where known) of NGC 1252 members from the literature. Not a single pair of stars can be found with matching parameters. Between all four sources the magnitudes of the stars extend from V = 6.62 to V = 17.97.
| α . | δ . | μα cos (δ) . | μδ . | ϖ . | |$v$|r . |
|---|---|---|---|---|---|
| ° . | ° . | |$\mathrm{mas\, yr^{-1}}$| . | |$\mathrm{mas\, yr^{-1}}$| . | mas . | |$\mathrm{km\, s^{-1}}$| . |
| Membersa in Kharchenko et al. (2013) | |||||
| 47.4215 | –57.6347 | –0.03 ± 0.05 | 4.90 ± 0.04 | 0.95 ± 0.03 | 0.5 ± 0.6b |
| 47.6764 | –57.7014 | –2.96 ± 0.03 | 15.57 ± 0.03 | 3.20 ± 0.02 | |
| 47.2933 | –57.7678 | –1.07 ± 0.06 | –13.19 ± 0.05 | 1.08 ± 0.03 | |
| 48.0644 | –57.6689 | –4.70 ± 0.05 | 3.90 ± 0.05 | 1.39 ± 0.03 | |
| 47.7155 | –57.6683 | 1.57 ± 0.05 | –1.88 ± 0.04 | 0.61 ± 0.03 | |
| 47.9065 | –57.5849 | 9.76 ± 0.15 | 3.23 ± 0.14 | 1.26 ± 0.07 | |
| 48.0170 | –57.7205 | 2.12 ± 0.05 | 9.79 ± 0.04 | 0.98 ± 0.02 | 31.4 ± 0.3c |
| 47.3650 | –57.6324 | –3.59 ± 0.10 | 12.80 ± 0.09 | 1.72 ± 0.05 | |
| 47.7089 | –57.7856 | 0.04 ± 0.05 | 6.32 ± 0.04 | 1.63 ± 0.03 | 20.3 ± 0.8b |
| 47.3982 | –57.8135 | 6.42 ± 0.04 | 4.39 ± 0.03 | 0.76 ± 0.02 | |
| 47.9903 | –57.6525 | 4.39 ± 0.14 | 9.04 ± 0.14 | 1.49 ± 0.07 | |
| Members in de la Fuente Marcos et al. (2013) | |||||
| 47.6605 | –57.7887 | 6.44 ± 0.05 | 7.61 ± 0.04 | 1.50 ± 0.02 | –4.4 ± 1.1b |
| 47.7356 | –57.7966 | 5.55 ± 0.04 | 11.25 ± 0.03 | 1.09 ± 0.02 | 5.3 ± 0.2c |
| 47.7498 | –57.6912 | 9.95 ± 0.08 | 9.81 ± 0.07 | 0.85 ± 0.05 | |
| 47.4953 | –57.7548 | 3.06 ± 0.10 | 10.20 ± 0.09 | 0.66 ± 0.05 | |
| 47.6336 | –57.6454 | 3.49 ± 0.05 | 5.74 ± 0.05 | 0.81 ± 0.03 | |
| 47.9003 | –57.6730 | 13.01 ± 0.03 | 6.05 ± 0.03 | 2.26 ± 0.02 | |
| 48.0170 | –57.7205 | 2.12 ± 0.05 | 9.79 ± 0.04 | 0.98 ± 0.02 | 31.4 ± 0.3c |
| 48.0104 | –57.6817 | 5.09 ± 0.07 | –0.90 ± 0.07 | 0.25 ± 0.04 | |
| Members in Pavani et al. (2001) | |||||
| 47.7089 | –57.7856 | 0.04 ± 0.05 | 6.32 ± 0.04 | 1.63 ± 0.03 | 20.3 ± 0.8b |
| 47.6868 | –57.7234 | –21.39 ± 0.04 | –44.09 ± 0.04 | 1.88 ± 0.02 | 20.1 ± 1.5b |
| 47.7680 | –57.7731 | –17.57 ± 0.05 | –18.16 ± 0.05 | 2.05 ± 0.03 | |
| 47.7356 | –57.7966 | 5.55 ± 0.04 | 11.25 ± 0.03 | 1.09 ± 0.02 | 5.3 ± 0.2c |
| 47.7498 | –57.7446 | 31.21 ± 0.03 | 17.01 ± 0.03 | 1.77 ± 0.02 | 43.3 ± 4.4b |
| 47.6764 | –57.7014 | –2.96 ± 0.03 | 15.57 ± 0.03 | 3.20 ± 0.02 | |
| 47.7083 | –57.7021 | 4.05 ± 0.07 | –69.89 ± 0.06 | 11.87 ± 0.04 | 54.0 ± 0.3b |
| Members in Bouchet & The (1983) | |||||
| 47.7083 | –57.7021 | 4.05 ± 0.07 | –69.89 ± 0.06 | 11.87 ± 0.04 | 54.0 ± 0.3b |
| 48.1091 | –57.7038 | 35.61 ± 0.04 | 1.30 ± 0.04 | 1.73 ± 0.02 | 50.8 ± 0.2b |
| 48.2607 | –57.8339 | 1.19 ± 0.07 | –4.57 ± 0.08 | 1.08 ± 0.05 | |
| 48.2768 | –57.6225 | 5.54 ± 0.05 | 17.82 ± 0.06 | 4.28 ± 0.03 | 30.8 ± 0.5b |
| 48.2507 | –57.5659 | 16.81 ± 0.04 | 4.41 ± 0.04 | 1.09 ± 0.02 | 30.8 ± 0.5b |
| 48.0351 | –57.5712 | 43.18 ± 0.06 | 15.34 ± 0.06 | 3.25 ± 0.03 | 7.6 ± 0.3b |
| 47.9307 | –57.5136 | –5.85 ± 0.04 | 8.20 ± 0.04 | 2.12 ± 0.02 | 19.5 ± 0.2b |
| 48.1921 | –57.3504 | –5.42 ± 0.06 | 3.69 ± 0.06 | 4.00 ± 0.03 | –12.6 ± 0.5b |
| 47.7845 | –57.1932 | –3.39 ± 0.09 | –26.14 ± 0.10 | 4.86 ± 0.05 | 7.0 ± 0.5b |
| 47.8202 | –57.1590 | 19.11 ± 0.24 | 19.46 ± 0.23 | 1.77 ± 0.13 | 4.3 ± 0.3b |
| 47.9257 | –56.9778 | –8.18 ± 0.04 | –7.17 ± 0.04 | 1.82 ± 0.02 | 13.3 ± 0.2b |
| 47.0998 | –57.0100 | 14.40 ± 0.04 | –13.60 ± 0.05 | 2.62 ± 0.03 | 5.6 ± 0.2b |
| 48.7182 | –57.8377 | –6.38 ± 0.08 | –15.96 ± 0.08 | 2.82 ± 0.05 | 105.3 ± 0.3b |
| α . | δ . | μα cos (δ) . | μδ . | ϖ . | |$v$|r . |
|---|---|---|---|---|---|
| ° . | ° . | |$\mathrm{mas\, yr^{-1}}$| . | |$\mathrm{mas\, yr^{-1}}$| . | mas . | |$\mathrm{km\, s^{-1}}$| . |
| Membersa in Kharchenko et al. (2013) | |||||
| 47.4215 | –57.6347 | –0.03 ± 0.05 | 4.90 ± 0.04 | 0.95 ± 0.03 | 0.5 ± 0.6b |
| 47.6764 | –57.7014 | –2.96 ± 0.03 | 15.57 ± 0.03 | 3.20 ± 0.02 | |
| 47.2933 | –57.7678 | –1.07 ± 0.06 | –13.19 ± 0.05 | 1.08 ± 0.03 | |
| 48.0644 | –57.6689 | –4.70 ± 0.05 | 3.90 ± 0.05 | 1.39 ± 0.03 | |
| 47.7155 | –57.6683 | 1.57 ± 0.05 | –1.88 ± 0.04 | 0.61 ± 0.03 | |
| 47.9065 | –57.5849 | 9.76 ± 0.15 | 3.23 ± 0.14 | 1.26 ± 0.07 | |
| 48.0170 | –57.7205 | 2.12 ± 0.05 | 9.79 ± 0.04 | 0.98 ± 0.02 | 31.4 ± 0.3c |
| 47.3650 | –57.6324 | –3.59 ± 0.10 | 12.80 ± 0.09 | 1.72 ± 0.05 | |
| 47.7089 | –57.7856 | 0.04 ± 0.05 | 6.32 ± 0.04 | 1.63 ± 0.03 | 20.3 ± 0.8b |
| 47.3982 | –57.8135 | 6.42 ± 0.04 | 4.39 ± 0.03 | 0.76 ± 0.02 | |
| 47.9903 | –57.6525 | 4.39 ± 0.14 | 9.04 ± 0.14 | 1.49 ± 0.07 | |
| Members in de la Fuente Marcos et al. (2013) | |||||
| 47.6605 | –57.7887 | 6.44 ± 0.05 | 7.61 ± 0.04 | 1.50 ± 0.02 | –4.4 ± 1.1b |
| 47.7356 | –57.7966 | 5.55 ± 0.04 | 11.25 ± 0.03 | 1.09 ± 0.02 | 5.3 ± 0.2c |
| 47.7498 | –57.6912 | 9.95 ± 0.08 | 9.81 ± 0.07 | 0.85 ± 0.05 | |
| 47.4953 | –57.7548 | 3.06 ± 0.10 | 10.20 ± 0.09 | 0.66 ± 0.05 | |
| 47.6336 | –57.6454 | 3.49 ± 0.05 | 5.74 ± 0.05 | 0.81 ± 0.03 | |
| 47.9003 | –57.6730 | 13.01 ± 0.03 | 6.05 ± 0.03 | 2.26 ± 0.02 | |
| 48.0170 | –57.7205 | 2.12 ± 0.05 | 9.79 ± 0.04 | 0.98 ± 0.02 | 31.4 ± 0.3c |
| 48.0104 | –57.6817 | 5.09 ± 0.07 | –0.90 ± 0.07 | 0.25 ± 0.04 | |
| Members in Pavani et al. (2001) | |||||
| 47.7089 | –57.7856 | 0.04 ± 0.05 | 6.32 ± 0.04 | 1.63 ± 0.03 | 20.3 ± 0.8b |
| 47.6868 | –57.7234 | –21.39 ± 0.04 | –44.09 ± 0.04 | 1.88 ± 0.02 | 20.1 ± 1.5b |
| 47.7680 | –57.7731 | –17.57 ± 0.05 | –18.16 ± 0.05 | 2.05 ± 0.03 | |
| 47.7356 | –57.7966 | 5.55 ± 0.04 | 11.25 ± 0.03 | 1.09 ± 0.02 | 5.3 ± 0.2c |
| 47.7498 | –57.7446 | 31.21 ± 0.03 | 17.01 ± 0.03 | 1.77 ± 0.02 | 43.3 ± 4.4b |
| 47.6764 | –57.7014 | –2.96 ± 0.03 | 15.57 ± 0.03 | 3.20 ± 0.02 | |
| 47.7083 | –57.7021 | 4.05 ± 0.07 | –69.89 ± 0.06 | 11.87 ± 0.04 | 54.0 ± 0.3b |
| Members in Bouchet & The (1983) | |||||
| 47.7083 | –57.7021 | 4.05 ± 0.07 | –69.89 ± 0.06 | 11.87 ± 0.04 | 54.0 ± 0.3b |
| 48.1091 | –57.7038 | 35.61 ± 0.04 | 1.30 ± 0.04 | 1.73 ± 0.02 | 50.8 ± 0.2b |
| 48.2607 | –57.8339 | 1.19 ± 0.07 | –4.57 ± 0.08 | 1.08 ± 0.05 | |
| 48.2768 | –57.6225 | 5.54 ± 0.05 | 17.82 ± 0.06 | 4.28 ± 0.03 | 30.8 ± 0.5b |
| 48.2507 | –57.5659 | 16.81 ± 0.04 | 4.41 ± 0.04 | 1.09 ± 0.02 | 30.8 ± 0.5b |
| 48.0351 | –57.5712 | 43.18 ± 0.06 | 15.34 ± 0.06 | 3.25 ± 0.03 | 7.6 ± 0.3b |
| 47.9307 | –57.5136 | –5.85 ± 0.04 | 8.20 ± 0.04 | 2.12 ± 0.02 | 19.5 ± 0.2b |
| 48.1921 | –57.3504 | –5.42 ± 0.06 | 3.69 ± 0.06 | 4.00 ± 0.03 | –12.6 ± 0.5b |
| 47.7845 | –57.1932 | –3.39 ± 0.09 | –26.14 ± 0.10 | 4.86 ± 0.05 | 7.0 ± 0.5b |
| 47.8202 | –57.1590 | 19.11 ± 0.24 | 19.46 ± 0.23 | 1.77 ± 0.13 | 4.3 ± 0.3b |
| 47.9257 | –56.9778 | –8.18 ± 0.04 | –7.17 ± 0.04 | 1.82 ± 0.02 | 13.3 ± 0.2b |
| 47.0998 | –57.0100 | 14.40 ± 0.04 | –13.60 ± 0.05 | 2.62 ± 0.03 | 5.6 ± 0.2b |
| 48.7182 | –57.8377 | –6.38 ± 0.08 | –15.96 ± 0.08 | 2.82 ± 0.05 | 105.3 ± 0.3b |
aOnly members with probability >0.8.
b|$v$|r from Gaia DR2.
c|$v$|r from GALAH.
Coordinates, proper motions, parallax, and radial velocity (where known) of NGC 1252 members from the literature. Not a single pair of stars can be found with matching parameters. Between all four sources the magnitudes of the stars extend from V = 6.62 to V = 17.97.
| α . | δ . | μα cos (δ) . | μδ . | ϖ . | |$v$|r . |
|---|---|---|---|---|---|
| ° . | ° . | |$\mathrm{mas\, yr^{-1}}$| . | |$\mathrm{mas\, yr^{-1}}$| . | mas . | |$\mathrm{km\, s^{-1}}$| . |
| Membersa in Kharchenko et al. (2013) | |||||
| 47.4215 | –57.6347 | –0.03 ± 0.05 | 4.90 ± 0.04 | 0.95 ± 0.03 | 0.5 ± 0.6b |
| 47.6764 | –57.7014 | –2.96 ± 0.03 | 15.57 ± 0.03 | 3.20 ± 0.02 | |
| 47.2933 | –57.7678 | –1.07 ± 0.06 | –13.19 ± 0.05 | 1.08 ± 0.03 | |
| 48.0644 | –57.6689 | –4.70 ± 0.05 | 3.90 ± 0.05 | 1.39 ± 0.03 | |
| 47.7155 | –57.6683 | 1.57 ± 0.05 | –1.88 ± 0.04 | 0.61 ± 0.03 | |
| 47.9065 | –57.5849 | 9.76 ± 0.15 | 3.23 ± 0.14 | 1.26 ± 0.07 | |
| 48.0170 | –57.7205 | 2.12 ± 0.05 | 9.79 ± 0.04 | 0.98 ± 0.02 | 31.4 ± 0.3c |
| 47.3650 | –57.6324 | –3.59 ± 0.10 | 12.80 ± 0.09 | 1.72 ± 0.05 | |
| 47.7089 | –57.7856 | 0.04 ± 0.05 | 6.32 ± 0.04 | 1.63 ± 0.03 | 20.3 ± 0.8b |
| 47.3982 | –57.8135 | 6.42 ± 0.04 | 4.39 ± 0.03 | 0.76 ± 0.02 | |
| 47.9903 | –57.6525 | 4.39 ± 0.14 | 9.04 ± 0.14 | 1.49 ± 0.07 | |
| Members in de la Fuente Marcos et al. (2013) | |||||
| 47.6605 | –57.7887 | 6.44 ± 0.05 | 7.61 ± 0.04 | 1.50 ± 0.02 | –4.4 ± 1.1b |
| 47.7356 | –57.7966 | 5.55 ± 0.04 | 11.25 ± 0.03 | 1.09 ± 0.02 | 5.3 ± 0.2c |
| 47.7498 | –57.6912 | 9.95 ± 0.08 | 9.81 ± 0.07 | 0.85 ± 0.05 | |
| 47.4953 | –57.7548 | 3.06 ± 0.10 | 10.20 ± 0.09 | 0.66 ± 0.05 | |
| 47.6336 | –57.6454 | 3.49 ± 0.05 | 5.74 ± 0.05 | 0.81 ± 0.03 | |
| 47.9003 | –57.6730 | 13.01 ± 0.03 | 6.05 ± 0.03 | 2.26 ± 0.02 | |
| 48.0170 | –57.7205 | 2.12 ± 0.05 | 9.79 ± 0.04 | 0.98 ± 0.02 | 31.4 ± 0.3c |
| 48.0104 | –57.6817 | 5.09 ± 0.07 | –0.90 ± 0.07 | 0.25 ± 0.04 | |
| Members in Pavani et al. (2001) | |||||
| 47.7089 | –57.7856 | 0.04 ± 0.05 | 6.32 ± 0.04 | 1.63 ± 0.03 | 20.3 ± 0.8b |
| 47.6868 | –57.7234 | –21.39 ± 0.04 | –44.09 ± 0.04 | 1.88 ± 0.02 | 20.1 ± 1.5b |
| 47.7680 | –57.7731 | –17.57 ± 0.05 | –18.16 ± 0.05 | 2.05 ± 0.03 | |
| 47.7356 | –57.7966 | 5.55 ± 0.04 | 11.25 ± 0.03 | 1.09 ± 0.02 | 5.3 ± 0.2c |
| 47.7498 | –57.7446 | 31.21 ± 0.03 | 17.01 ± 0.03 | 1.77 ± 0.02 | 43.3 ± 4.4b |
| 47.6764 | –57.7014 | –2.96 ± 0.03 | 15.57 ± 0.03 | 3.20 ± 0.02 | |
| 47.7083 | –57.7021 | 4.05 ± 0.07 | –69.89 ± 0.06 | 11.87 ± 0.04 | 54.0 ± 0.3b |
| Members in Bouchet & The (1983) | |||||
| 47.7083 | –57.7021 | 4.05 ± 0.07 | –69.89 ± 0.06 | 11.87 ± 0.04 | 54.0 ± 0.3b |
| 48.1091 | –57.7038 | 35.61 ± 0.04 | 1.30 ± 0.04 | 1.73 ± 0.02 | 50.8 ± 0.2b |
| 48.2607 | –57.8339 | 1.19 ± 0.07 | –4.57 ± 0.08 | 1.08 ± 0.05 | |
| 48.2768 | –57.6225 | 5.54 ± 0.05 | 17.82 ± 0.06 | 4.28 ± 0.03 | 30.8 ± 0.5b |
| 48.2507 | –57.5659 | 16.81 ± 0.04 | 4.41 ± 0.04 | 1.09 ± 0.02 | 30.8 ± 0.5b |
| 48.0351 | –57.5712 | 43.18 ± 0.06 | 15.34 ± 0.06 | 3.25 ± 0.03 | 7.6 ± 0.3b |
| 47.9307 | –57.5136 | –5.85 ± 0.04 | 8.20 ± 0.04 | 2.12 ± 0.02 | 19.5 ± 0.2b |
| 48.1921 | –57.3504 | –5.42 ± 0.06 | 3.69 ± 0.06 | 4.00 ± 0.03 | –12.6 ± 0.5b |
| 47.7845 | –57.1932 | –3.39 ± 0.09 | –26.14 ± 0.10 | 4.86 ± 0.05 | 7.0 ± 0.5b |
| 47.8202 | –57.1590 | 19.11 ± 0.24 | 19.46 ± 0.23 | 1.77 ± 0.13 | 4.3 ± 0.3b |
| 47.9257 | –56.9778 | –8.18 ± 0.04 | –7.17 ± 0.04 | 1.82 ± 0.02 | 13.3 ± 0.2b |
| 47.0998 | –57.0100 | 14.40 ± 0.04 | –13.60 ± 0.05 | 2.62 ± 0.03 | 5.6 ± 0.2b |
| 48.7182 | –57.8377 | –6.38 ± 0.08 | –15.96 ± 0.08 | 2.82 ± 0.05 | 105.3 ± 0.3b |
| α . | δ . | μα cos (δ) . | μδ . | ϖ . | |$v$|r . |
|---|---|---|---|---|---|
| ° . | ° . | |$\mathrm{mas\, yr^{-1}}$| . | |$\mathrm{mas\, yr^{-1}}$| . | mas . | |$\mathrm{km\, s^{-1}}$| . |
| Membersa in Kharchenko et al. (2013) | |||||
| 47.4215 | –57.6347 | –0.03 ± 0.05 | 4.90 ± 0.04 | 0.95 ± 0.03 | 0.5 ± 0.6b |
| 47.6764 | –57.7014 | –2.96 ± 0.03 | 15.57 ± 0.03 | 3.20 ± 0.02 | |
| 47.2933 | –57.7678 | –1.07 ± 0.06 | –13.19 ± 0.05 | 1.08 ± 0.03 | |
| 48.0644 | –57.6689 | –4.70 ± 0.05 | 3.90 ± 0.05 | 1.39 ± 0.03 | |
| 47.7155 | –57.6683 | 1.57 ± 0.05 | –1.88 ± 0.04 | 0.61 ± 0.03 | |
| 47.9065 | –57.5849 | 9.76 ± 0.15 | 3.23 ± 0.14 | 1.26 ± 0.07 | |
| 48.0170 | –57.7205 | 2.12 ± 0.05 | 9.79 ± 0.04 | 0.98 ± 0.02 | 31.4 ± 0.3c |
| 47.3650 | –57.6324 | –3.59 ± 0.10 | 12.80 ± 0.09 | 1.72 ± 0.05 | |
| 47.7089 | –57.7856 | 0.04 ± 0.05 | 6.32 ± 0.04 | 1.63 ± 0.03 | 20.3 ± 0.8b |
| 47.3982 | –57.8135 | 6.42 ± 0.04 | 4.39 ± 0.03 | 0.76 ± 0.02 | |
| 47.9903 | –57.6525 | 4.39 ± 0.14 | 9.04 ± 0.14 | 1.49 ± 0.07 | |
| Members in de la Fuente Marcos et al. (2013) | |||||
| 47.6605 | –57.7887 | 6.44 ± 0.05 | 7.61 ± 0.04 | 1.50 ± 0.02 | –4.4 ± 1.1b |
| 47.7356 | –57.7966 | 5.55 ± 0.04 | 11.25 ± 0.03 | 1.09 ± 0.02 | 5.3 ± 0.2c |
| 47.7498 | –57.6912 | 9.95 ± 0.08 | 9.81 ± 0.07 | 0.85 ± 0.05 | |
| 47.4953 | –57.7548 | 3.06 ± 0.10 | 10.20 ± 0.09 | 0.66 ± 0.05 | |
| 47.6336 | –57.6454 | 3.49 ± 0.05 | 5.74 ± 0.05 | 0.81 ± 0.03 | |
| 47.9003 | –57.6730 | 13.01 ± 0.03 | 6.05 ± 0.03 | 2.26 ± 0.02 | |
| 48.0170 | –57.7205 | 2.12 ± 0.05 | 9.79 ± 0.04 | 0.98 ± 0.02 | 31.4 ± 0.3c |
| 48.0104 | –57.6817 | 5.09 ± 0.07 | –0.90 ± 0.07 | 0.25 ± 0.04 | |
| Members in Pavani et al. (2001) | |||||
| 47.7089 | –57.7856 | 0.04 ± 0.05 | 6.32 ± 0.04 | 1.63 ± 0.03 | 20.3 ± 0.8b |
| 47.6868 | –57.7234 | –21.39 ± 0.04 | –44.09 ± 0.04 | 1.88 ± 0.02 | 20.1 ± 1.5b |
| 47.7680 | –57.7731 | –17.57 ± 0.05 | –18.16 ± 0.05 | 2.05 ± 0.03 | |
| 47.7356 | –57.7966 | 5.55 ± 0.04 | 11.25 ± 0.03 | 1.09 ± 0.02 | 5.3 ± 0.2c |
| 47.7498 | –57.7446 | 31.21 ± 0.03 | 17.01 ± 0.03 | 1.77 ± 0.02 | 43.3 ± 4.4b |
| 47.6764 | –57.7014 | –2.96 ± 0.03 | 15.57 ± 0.03 | 3.20 ± 0.02 | |
| 47.7083 | –57.7021 | 4.05 ± 0.07 | –69.89 ± 0.06 | 11.87 ± 0.04 | 54.0 ± 0.3b |
| Members in Bouchet & The (1983) | |||||
| 47.7083 | –57.7021 | 4.05 ± 0.07 | –69.89 ± 0.06 | 11.87 ± 0.04 | 54.0 ± 0.3b |
| 48.1091 | –57.7038 | 35.61 ± 0.04 | 1.30 ± 0.04 | 1.73 ± 0.02 | 50.8 ± 0.2b |
| 48.2607 | –57.8339 | 1.19 ± 0.07 | –4.57 ± 0.08 | 1.08 ± 0.05 | |
| 48.2768 | –57.6225 | 5.54 ± 0.05 | 17.82 ± 0.06 | 4.28 ± 0.03 | 30.8 ± 0.5b |
| 48.2507 | –57.5659 | 16.81 ± 0.04 | 4.41 ± 0.04 | 1.09 ± 0.02 | 30.8 ± 0.5b |
| 48.0351 | –57.5712 | 43.18 ± 0.06 | 15.34 ± 0.06 | 3.25 ± 0.03 | 7.6 ± 0.3b |
| 47.9307 | –57.5136 | –5.85 ± 0.04 | 8.20 ± 0.04 | 2.12 ± 0.02 | 19.5 ± 0.2b |
| 48.1921 | –57.3504 | –5.42 ± 0.06 | 3.69 ± 0.06 | 4.00 ± 0.03 | –12.6 ± 0.5b |
| 47.7845 | –57.1932 | –3.39 ± 0.09 | –26.14 ± 0.10 | 4.86 ± 0.05 | 7.0 ± 0.5b |
| 47.8202 | –57.1590 | 19.11 ± 0.24 | 19.46 ± 0.23 | 1.77 ± 0.13 | 4.3 ± 0.3b |
| 47.9257 | –56.9778 | –8.18 ± 0.04 | –7.17 ± 0.04 | 1.82 ± 0.02 | 13.3 ± 0.2b |
| 47.0998 | –57.0100 | 14.40 ± 0.04 | –13.60 ± 0.05 | 2.62 ± 0.03 | 5.6 ± 0.2b |
| 48.7182 | –57.8377 | –6.38 ± 0.08 | –15.96 ± 0.08 | 2.82 ± 0.05 | 105.3 ± 0.3b |
aOnly members with probability >0.8.
b|$v$|r from Gaia DR2.
c|$v$|r from GALAH.
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