Coordinates, proper motions, parallax, and radial velocity (where known) of NGC 7772 members from the literature. Not a single pair of stars can be found with matching parameters. Between both sources the magnitudes of the stars extend from V = 11.08 to V = 18.00.
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) | |||||
357.9917 | 16.2920 | 17.13 ± 0.05 | –8.65 ± 0.02 | 1.39 ± 0.03 | |
357.8054 | 16.1146 | 6.94 ± 0.34 | –2.56 ± 0.14 | 1.30 ± 0.16 | |
357.5001 | 16.1331 | 12.52 ± 0.09 | –10.44 ± 0.04 | 2.77 ± 0.04 | 22.7 ± 1.7b |
358.2582 | 16.4424 | 18.28 ± 0.13 | –14.25 ± 0.06 | 1.03 ± 0.07 | |
357.9434 | 16.2490 | 12.45 ± 0.05 | –7.38 ± 0.02 | 1.88 ± 0.03 | |
357.9288 | 16.2352 | 7.30 ± 0.08 | –8.65 ± 0.04 | 0.52 ± 0.04 | 22.1 ± 0.3b |
357.9052 | 15.9786 | 11.59 ± 0.10 | –7.66 ± 0.04 | 1.05 ± 0.05 | |
358.0828 | 16.2812 | 10.42 ± 0.30 | –6.91 ± 0.18 | 1.53 ± 0.15 | |
357.9428 | 16.2398 | 12.50 ± 0.07 | –7.25 ± 0.04 | 1.95 ± 0.04 | –63.4 ± 0.1c |
358.3233 | 16.0572 | 16.19 ± 0.09 | –9.59 ± 0.04 | 1.03 ± 0.05 | |
Members in Carraro (2002) | |||||
357.9428 | 16.2398 | 12.50 ± 0.07 | –7.25 ± 0.04 | 1.95 ± 0.04 | –63.4 ± 0.1c |
357.9690 | 16.1878 | 6.75 ± 0.16 | –38.26 ± 0.08 | 5.48 ± 0.09 | –20.1 ± 1.2b |
357.9129 | 16.3036 | –16.76 ± 0.06 | –31.33 ± 0.03 | 2.04 ± 0.03 | |
357.9506 | 16.2513 | 8.65 ± 0.06 | –10.52 ± 0.03 | 1.02 ± 0.03 | –69.9 ± 1.3b |
357.9434 | 16.2490 | 12.45 ± 0.05 | –7.38 ± 0.02 | 1.88 ± 0.03 | |
357.8977 | 16.2136 | –6.48 ± 0.05 | –18.50 ± 0.02 | 0.64 ± 0.03 | |
357.9503 | 16.2333 | 0.52 ± 0.05 | –2.54 ± 0.03 | 2.34 ± 0.03 | 18.8 ± 0.2c |
357.9917 | 16.2920 | 17.13 ± 0.05 | –8.65 ± 0.02 | 1.39 ± 0.03 | |
357.9367 | 16.2454 | 12.56 ± 0.05 | 5.86 ± 0.03 | 1.50 ± 0.03 | |
357.9538 | 16.1833 | –4.48 ± 0.05 | –6.55 ± 0.03 | 1.59 ± 0.03 | –37.2 ± 0.1c |
357.9056 | 16.3006 | 2.74 ± 0.08 | 0.49 ± 0.04 | 0.48 ± 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 Kharchenko et al. (2013) | |||||
357.9917 | 16.2920 | 17.13 ± 0.05 | –8.65 ± 0.02 | 1.39 ± 0.03 | |
357.8054 | 16.1146 | 6.94 ± 0.34 | –2.56 ± 0.14 | 1.30 ± 0.16 | |
357.5001 | 16.1331 | 12.52 ± 0.09 | –10.44 ± 0.04 | 2.77 ± 0.04 | 22.7 ± 1.7b |
358.2582 | 16.4424 | 18.28 ± 0.13 | –14.25 ± 0.06 | 1.03 ± 0.07 | |
357.9434 | 16.2490 | 12.45 ± 0.05 | –7.38 ± 0.02 | 1.88 ± 0.03 | |
357.9288 | 16.2352 | 7.30 ± 0.08 | –8.65 ± 0.04 | 0.52 ± 0.04 | 22.1 ± 0.3b |
357.9052 | 15.9786 | 11.59 ± 0.10 | –7.66 ± 0.04 | 1.05 ± 0.05 | |
358.0828 | 16.2812 | 10.42 ± 0.30 | –6.91 ± 0.18 | 1.53 ± 0.15 | |
357.9428 | 16.2398 | 12.50 ± 0.07 | –7.25 ± 0.04 | 1.95 ± 0.04 | –63.4 ± 0.1c |
358.3233 | 16.0572 | 16.19 ± 0.09 | –9.59 ± 0.04 | 1.03 ± 0.05 | |
Members in Carraro (2002) | |||||
357.9428 | 16.2398 | 12.50 ± 0.07 | –7.25 ± 0.04 | 1.95 ± 0.04 | –63.4 ± 0.1c |
357.9690 | 16.1878 | 6.75 ± 0.16 | –38.26 ± 0.08 | 5.48 ± 0.09 | –20.1 ± 1.2b |
357.9129 | 16.3036 | –16.76 ± 0.06 | –31.33 ± 0.03 | 2.04 ± 0.03 | |
357.9506 | 16.2513 | 8.65 ± 0.06 | –10.52 ± 0.03 | 1.02 ± 0.03 | –69.9 ± 1.3b |
357.9434 | 16.2490 | 12.45 ± 0.05 | –7.38 ± 0.02 | 1.88 ± 0.03 | |
357.8977 | 16.2136 | –6.48 ± 0.05 | –18.50 ± 0.02 | 0.64 ± 0.03 | |
357.9503 | 16.2333 | 0.52 ± 0.05 | –2.54 ± 0.03 | 2.34 ± 0.03 | 18.8 ± 0.2c |
357.9917 | 16.2920 | 17.13 ± 0.05 | –8.65 ± 0.02 | 1.39 ± 0.03 | |
357.9367 | 16.2454 | 12.56 ± 0.05 | 5.86 ± 0.03 | 1.50 ± 0.03 | |
357.9538 | 16.1833 | –4.48 ± 0.05 | –6.55 ± 0.03 | 1.59 ± 0.03 | –37.2 ± 0.1c |
357.9056 | 16.3006 | 2.74 ± 0.08 | 0.49 ± 0.04 | 0.48 ± 0.04 |
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 7772 members from the literature. Not a single pair of stars can be found with matching parameters. Between both sources the magnitudes of the stars extend from V = 11.08 to V = 18.00.
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) | |||||
357.9917 | 16.2920 | 17.13 ± 0.05 | –8.65 ± 0.02 | 1.39 ± 0.03 | |
357.8054 | 16.1146 | 6.94 ± 0.34 | –2.56 ± 0.14 | 1.30 ± 0.16 | |
357.5001 | 16.1331 | 12.52 ± 0.09 | –10.44 ± 0.04 | 2.77 ± 0.04 | 22.7 ± 1.7b |
358.2582 | 16.4424 | 18.28 ± 0.13 | –14.25 ± 0.06 | 1.03 ± 0.07 | |
357.9434 | 16.2490 | 12.45 ± 0.05 | –7.38 ± 0.02 | 1.88 ± 0.03 | |
357.9288 | 16.2352 | 7.30 ± 0.08 | –8.65 ± 0.04 | 0.52 ± 0.04 | 22.1 ± 0.3b |
357.9052 | 15.9786 | 11.59 ± 0.10 | –7.66 ± 0.04 | 1.05 ± 0.05 | |
358.0828 | 16.2812 | 10.42 ± 0.30 | –6.91 ± 0.18 | 1.53 ± 0.15 | |
357.9428 | 16.2398 | 12.50 ± 0.07 | –7.25 ± 0.04 | 1.95 ± 0.04 | –63.4 ± 0.1c |
358.3233 | 16.0572 | 16.19 ± 0.09 | –9.59 ± 0.04 | 1.03 ± 0.05 | |
Members in Carraro (2002) | |||||
357.9428 | 16.2398 | 12.50 ± 0.07 | –7.25 ± 0.04 | 1.95 ± 0.04 | –63.4 ± 0.1c |
357.9690 | 16.1878 | 6.75 ± 0.16 | –38.26 ± 0.08 | 5.48 ± 0.09 | –20.1 ± 1.2b |
357.9129 | 16.3036 | –16.76 ± 0.06 | –31.33 ± 0.03 | 2.04 ± 0.03 | |
357.9506 | 16.2513 | 8.65 ± 0.06 | –10.52 ± 0.03 | 1.02 ± 0.03 | –69.9 ± 1.3b |
357.9434 | 16.2490 | 12.45 ± 0.05 | –7.38 ± 0.02 | 1.88 ± 0.03 | |
357.8977 | 16.2136 | –6.48 ± 0.05 | –18.50 ± 0.02 | 0.64 ± 0.03 | |
357.9503 | 16.2333 | 0.52 ± 0.05 | –2.54 ± 0.03 | 2.34 ± 0.03 | 18.8 ± 0.2c |
357.9917 | 16.2920 | 17.13 ± 0.05 | –8.65 ± 0.02 | 1.39 ± 0.03 | |
357.9367 | 16.2454 | 12.56 ± 0.05 | 5.86 ± 0.03 | 1.50 ± 0.03 | |
357.9538 | 16.1833 | –4.48 ± 0.05 | –6.55 ± 0.03 | 1.59 ± 0.03 | –37.2 ± 0.1c |
357.9056 | 16.3006 | 2.74 ± 0.08 | 0.49 ± 0.04 | 0.48 ± 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 Kharchenko et al. (2013) | |||||
357.9917 | 16.2920 | 17.13 ± 0.05 | –8.65 ± 0.02 | 1.39 ± 0.03 | |
357.8054 | 16.1146 | 6.94 ± 0.34 | –2.56 ± 0.14 | 1.30 ± 0.16 | |
357.5001 | 16.1331 | 12.52 ± 0.09 | –10.44 ± 0.04 | 2.77 ± 0.04 | 22.7 ± 1.7b |
358.2582 | 16.4424 | 18.28 ± 0.13 | –14.25 ± 0.06 | 1.03 ± 0.07 | |
357.9434 | 16.2490 | 12.45 ± 0.05 | –7.38 ± 0.02 | 1.88 ± 0.03 | |
357.9288 | 16.2352 | 7.30 ± 0.08 | –8.65 ± 0.04 | 0.52 ± 0.04 | 22.1 ± 0.3b |
357.9052 | 15.9786 | 11.59 ± 0.10 | –7.66 ± 0.04 | 1.05 ± 0.05 | |
358.0828 | 16.2812 | 10.42 ± 0.30 | –6.91 ± 0.18 | 1.53 ± 0.15 | |
357.9428 | 16.2398 | 12.50 ± 0.07 | –7.25 ± 0.04 | 1.95 ± 0.04 | –63.4 ± 0.1c |
358.3233 | 16.0572 | 16.19 ± 0.09 | –9.59 ± 0.04 | 1.03 ± 0.05 | |
Members in Carraro (2002) | |||||
357.9428 | 16.2398 | 12.50 ± 0.07 | –7.25 ± 0.04 | 1.95 ± 0.04 | –63.4 ± 0.1c |
357.9690 | 16.1878 | 6.75 ± 0.16 | –38.26 ± 0.08 | 5.48 ± 0.09 | –20.1 ± 1.2b |
357.9129 | 16.3036 | –16.76 ± 0.06 | –31.33 ± 0.03 | 2.04 ± 0.03 | |
357.9506 | 16.2513 | 8.65 ± 0.06 | –10.52 ± 0.03 | 1.02 ± 0.03 | –69.9 ± 1.3b |
357.9434 | 16.2490 | 12.45 ± 0.05 | –7.38 ± 0.02 | 1.88 ± 0.03 | |
357.8977 | 16.2136 | –6.48 ± 0.05 | –18.50 ± 0.02 | 0.64 ± 0.03 | |
357.9503 | 16.2333 | 0.52 ± 0.05 | –2.54 ± 0.03 | 2.34 ± 0.03 | 18.8 ± 0.2c |
357.9917 | 16.2920 | 17.13 ± 0.05 | –8.65 ± 0.02 | 1.39 ± 0.03 | |
357.9367 | 16.2454 | 12.56 ± 0.05 | 5.86 ± 0.03 | 1.50 ± 0.03 | |
357.9538 | 16.1833 | –4.48 ± 0.05 | –6.55 ± 0.03 | 1.59 ± 0.03 | –37.2 ± 0.1c |
357.9056 | 16.3006 | 2.74 ± 0.08 | 0.49 ± 0.04 | 0.48 ± 0.04 |
aOnly members with probability >0.8.
b|$v$|r from Gaia DR2.
c|$v$|r from GALAH.
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