Coordinates, proper motions, parallax, and radial velocity (where known) of NGC 7826 members from the literature. Not a single pair of stars can be found with matching parameters. The magnitudes of the stars extend from V = 9.72 to V = 16.67.
α . | δ . | μα cos (δ) . | μδ . | ϖ . | |$v$|r . |
---|---|---|---|---|---|
° . | ° . | |$\mathrm{mas\, yr^{-1}}$| . | |$\mathrm{mas\, yr^{-1}}$| . | mas . | |$\mathrm{km\, s^{-1}}$| . |
Membersa in Dias et al. (2002, 2014) | |||||
1.3897 | –20.8588 | 12.26 ± 0.12 | 2.83 ± 0.07 | 0.72 ± 0.07 | |
1.1267 | –20.6970 | 46.70 ± 0.09 | –5.49 ± 0.06 | 3.22 ± 0.06 | –1.1 ± 0.2b |
1.2085 | –20.6567 | 25.99 ± 0.06 | –11.67 ± 0.04 | 1.30 ± 0.03 | |
1.2711 | –20.6347 | 15.25 ± 0.07 | –8.40 ± 0.05 | 0.36 ± 0.04 | 77.3 ± 0.1c |
1.2949 | –20.7413 | 14.65 ± 0.10 | 1.17 ± 0.06 | 1.18 ± 0.05 | |
1.2976 | –20.6020 | 19.74 ± 0.05 | 6.47 ± 0.03 | 0.79 ± 0.03 | –17.8 ± 0.1c |
1.3595 | –20.7226 | 38.34 ± 0.12 | 5.27 ± 0.06 | 3.39 ± 0.05 | 16.3 ± 0.7b |
1.3745 | –20.6056 | 27.03 ± 0.07 | –5.63 ± 0.04 | 3.53 ± 0.04 | –2.9 ± 0.1c |
1.4658 | –20.7048 | 16.05 ± 0.05 | –5.44 ± 0.04 | 0.92 ± 0.04 | |
1.2480 | –20.5623 | 18.41 ± 0.07 | –8.65 ± 0.05 | 1.99 ± 0.04 | 12.9 ± 1.1b |
1.4210 | –20.5883 | 12.84 ± 0.08 | 1.43 ± 0.04 | 2.54 ± 0.04 |
α . | δ . | μα cos (δ) . | μδ . | ϖ . | |$v$|r . |
---|---|---|---|---|---|
° . | ° . | |$\mathrm{mas\, yr^{-1}}$| . | |$\mathrm{mas\, yr^{-1}}$| . | mas . | |$\mathrm{km\, s^{-1}}$| . |
Membersa in Dias et al. (2002, 2014) | |||||
1.3897 | –20.8588 | 12.26 ± 0.12 | 2.83 ± 0.07 | 0.72 ± 0.07 | |
1.1267 | –20.6970 | 46.70 ± 0.09 | –5.49 ± 0.06 | 3.22 ± 0.06 | –1.1 ± 0.2b |
1.2085 | –20.6567 | 25.99 ± 0.06 | –11.67 ± 0.04 | 1.30 ± 0.03 | |
1.2711 | –20.6347 | 15.25 ± 0.07 | –8.40 ± 0.05 | 0.36 ± 0.04 | 77.3 ± 0.1c |
1.2949 | –20.7413 | 14.65 ± 0.10 | 1.17 ± 0.06 | 1.18 ± 0.05 | |
1.2976 | –20.6020 | 19.74 ± 0.05 | 6.47 ± 0.03 | 0.79 ± 0.03 | –17.8 ± 0.1c |
1.3595 | –20.7226 | 38.34 ± 0.12 | 5.27 ± 0.06 | 3.39 ± 0.05 | 16.3 ± 0.7b |
1.3745 | –20.6056 | 27.03 ± 0.07 | –5.63 ± 0.04 | 3.53 ± 0.04 | –2.9 ± 0.1c |
1.4658 | –20.7048 | 16.05 ± 0.05 | –5.44 ± 0.04 | 0.92 ± 0.04 | |
1.2480 | –20.5623 | 18.41 ± 0.07 | –8.65 ± 0.05 | 1.99 ± 0.04 | 12.9 ± 1.1b |
1.4210 | –20.5883 | 12.84 ± 0.08 | 1.43 ± 0.04 | 2.54 ± 0.04 |
aOnly members with probability >0.9.
b|$v$|r from Gaia DR2.
c|$v$|r from GALAH.
Coordinates, proper motions, parallax, and radial velocity (where known) of NGC 7826 members from the literature. Not a single pair of stars can be found with matching parameters. The magnitudes of the stars extend from V = 9.72 to V = 16.67.
α . | δ . | μα cos (δ) . | μδ . | ϖ . | |$v$|r . |
---|---|---|---|---|---|
° . | ° . | |$\mathrm{mas\, yr^{-1}}$| . | |$\mathrm{mas\, yr^{-1}}$| . | mas . | |$\mathrm{km\, s^{-1}}$| . |
Membersa in Dias et al. (2002, 2014) | |||||
1.3897 | –20.8588 | 12.26 ± 0.12 | 2.83 ± 0.07 | 0.72 ± 0.07 | |
1.1267 | –20.6970 | 46.70 ± 0.09 | –5.49 ± 0.06 | 3.22 ± 0.06 | –1.1 ± 0.2b |
1.2085 | –20.6567 | 25.99 ± 0.06 | –11.67 ± 0.04 | 1.30 ± 0.03 | |
1.2711 | –20.6347 | 15.25 ± 0.07 | –8.40 ± 0.05 | 0.36 ± 0.04 | 77.3 ± 0.1c |
1.2949 | –20.7413 | 14.65 ± 0.10 | 1.17 ± 0.06 | 1.18 ± 0.05 | |
1.2976 | –20.6020 | 19.74 ± 0.05 | 6.47 ± 0.03 | 0.79 ± 0.03 | –17.8 ± 0.1c |
1.3595 | –20.7226 | 38.34 ± 0.12 | 5.27 ± 0.06 | 3.39 ± 0.05 | 16.3 ± 0.7b |
1.3745 | –20.6056 | 27.03 ± 0.07 | –5.63 ± 0.04 | 3.53 ± 0.04 | –2.9 ± 0.1c |
1.4658 | –20.7048 | 16.05 ± 0.05 | –5.44 ± 0.04 | 0.92 ± 0.04 | |
1.2480 | –20.5623 | 18.41 ± 0.07 | –8.65 ± 0.05 | 1.99 ± 0.04 | 12.9 ± 1.1b |
1.4210 | –20.5883 | 12.84 ± 0.08 | 1.43 ± 0.04 | 2.54 ± 0.04 |
α . | δ . | μα cos (δ) . | μδ . | ϖ . | |$v$|r . |
---|---|---|---|---|---|
° . | ° . | |$\mathrm{mas\, yr^{-1}}$| . | |$\mathrm{mas\, yr^{-1}}$| . | mas . | |$\mathrm{km\, s^{-1}}$| . |
Membersa in Dias et al. (2002, 2014) | |||||
1.3897 | –20.8588 | 12.26 ± 0.12 | 2.83 ± 0.07 | 0.72 ± 0.07 | |
1.1267 | –20.6970 | 46.70 ± 0.09 | –5.49 ± 0.06 | 3.22 ± 0.06 | –1.1 ± 0.2b |
1.2085 | –20.6567 | 25.99 ± 0.06 | –11.67 ± 0.04 | 1.30 ± 0.03 | |
1.2711 | –20.6347 | 15.25 ± 0.07 | –8.40 ± 0.05 | 0.36 ± 0.04 | 77.3 ± 0.1c |
1.2949 | –20.7413 | 14.65 ± 0.10 | 1.17 ± 0.06 | 1.18 ± 0.05 | |
1.2976 | –20.6020 | 19.74 ± 0.05 | 6.47 ± 0.03 | 0.79 ± 0.03 | –17.8 ± 0.1c |
1.3595 | –20.7226 | 38.34 ± 0.12 | 5.27 ± 0.06 | 3.39 ± 0.05 | 16.3 ± 0.7b |
1.3745 | –20.6056 | 27.03 ± 0.07 | –5.63 ± 0.04 | 3.53 ± 0.04 | –2.9 ± 0.1c |
1.4658 | –20.7048 | 16.05 ± 0.05 | –5.44 ± 0.04 | 0.92 ± 0.04 | |
1.2480 | –20.5623 | 18.41 ± 0.07 | –8.65 ± 0.05 | 1.99 ± 0.04 | 12.9 ± 1.1b |
1.4210 | –20.5883 | 12.84 ± 0.08 | 1.43 ± 0.04 | 2.54 ± 0.04 |
aOnly members with probability >0.9.
b|$v$|r from Gaia DR2.
c|$v$|r from GALAH.
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