Coordinates, proper motions, parallax, and radial velocity (where known) of NGC 6994 members from the literature. Not a single pair of stars can be found with matching parameters. The magnitudes of the stars extend from V = 10.35 to V = 19.53.
| α . | δ . | μα cos (δ) . | μδ . | ϖ . | |$v$|r . |
|---|---|---|---|---|---|
| ° . | ° . | |$\mathrm{mas\, yr^{-1}}$| . | |$\mathrm{mas\, yr^{-1}}$| . | mas . | |$\mathrm{km\, s^{-1}}$| . |
| Members in Bassino et al. (2000) | |||||
| 314.7366 | –12.6418 | 7.33 ± 0.07 | –15.55 ± 0.05 | 1.41 ± 0.04 | –26.2 ± 0.2a |
| 314.7401 | –12.6294 | 18.41 ± 0.07 | –7.72 ± 0.06 | 2.66 ± 0.05 | –53.1 ± 0.7a |
| 314.7283 | –12.6345 | 2.05 ± 0.09 | –10.80 ± 0.07 | 3.11 ± 0.06 | –8.5 ± 0.6a |
| 314.7222 | –12.6318 | 4.61 ± 0.07 | –7.03 ± 0.05 | 1.52 ± 0.04 | –20.8 ± 0.6a |
| 314.8046 | –12.6706 | –21.38 ± 0.05 | –9.39 ± 0.03 | 1.18 ± 0.03 | |
| 314.7781 | –12.5914 | 3.50 ± 0.05 | –6.02 ± 0.03 | 0.80 ± 0.03 | –11.6 ± 0.1b |
| 314.7776 | –12.5777 | –11.40 ± 0.07 | 1.19 ± 0.05 | 1.91 ± 0.05 | |
| 314.7423 | –12.5768 | –4.60 ± 0.04 | –5.57 ± 0.03 | 0.83 ± 0.03 | |
| 314.7237 | –12.5765 | –4.16 ± 0.04 | –6.62 ± 0.03 | 0.33 ± 0.03 | 51.5 ± 0.1b |
| 314.7378 | –12.5785 | –5.53 ± 0.35 | 2.55 ± 0.23 | 1.78 ± 0.23 | |
| 314.7487 | –12.6955 | 16.82 ± 0.07 | 7.75 ± 0.04 | 1.43 ± 0.04 | –28.2 ± 1.6a |
| α . | δ . | μα cos (δ) . | μδ . | ϖ . | |$v$|r . |
|---|---|---|---|---|---|
| ° . | ° . | |$\mathrm{mas\, yr^{-1}}$| . | |$\mathrm{mas\, yr^{-1}}$| . | mas . | |$\mathrm{km\, s^{-1}}$| . |
| Members in Bassino et al. (2000) | |||||
| 314.7366 | –12.6418 | 7.33 ± 0.07 | –15.55 ± 0.05 | 1.41 ± 0.04 | –26.2 ± 0.2a |
| 314.7401 | –12.6294 | 18.41 ± 0.07 | –7.72 ± 0.06 | 2.66 ± 0.05 | –53.1 ± 0.7a |
| 314.7283 | –12.6345 | 2.05 ± 0.09 | –10.80 ± 0.07 | 3.11 ± 0.06 | –8.5 ± 0.6a |
| 314.7222 | –12.6318 | 4.61 ± 0.07 | –7.03 ± 0.05 | 1.52 ± 0.04 | –20.8 ± 0.6a |
| 314.8046 | –12.6706 | –21.38 ± 0.05 | –9.39 ± 0.03 | 1.18 ± 0.03 | |
| 314.7781 | –12.5914 | 3.50 ± 0.05 | –6.02 ± 0.03 | 0.80 ± 0.03 | –11.6 ± 0.1b |
| 314.7776 | –12.5777 | –11.40 ± 0.07 | 1.19 ± 0.05 | 1.91 ± 0.05 | |
| 314.7423 | –12.5768 | –4.60 ± 0.04 | –5.57 ± 0.03 | 0.83 ± 0.03 | |
| 314.7237 | –12.5765 | –4.16 ± 0.04 | –6.62 ± 0.03 | 0.33 ± 0.03 | 51.5 ± 0.1b |
| 314.7378 | –12.5785 | –5.53 ± 0.35 | 2.55 ± 0.23 | 1.78 ± 0.23 | |
| 314.7487 | –12.6955 | 16.82 ± 0.07 | 7.75 ± 0.04 | 1.43 ± 0.04 | –28.2 ± 1.6a |
a|$v$|r from Gaia DR2.
b|$v$|r from GALAH.
Coordinates, proper motions, parallax, and radial velocity (where known) of NGC 6994 members from the literature. Not a single pair of stars can be found with matching parameters. The magnitudes of the stars extend from V = 10.35 to V = 19.53.
| α . | δ . | μα cos (δ) . | μδ . | ϖ . | |$v$|r . |
|---|---|---|---|---|---|
| ° . | ° . | |$\mathrm{mas\, yr^{-1}}$| . | |$\mathrm{mas\, yr^{-1}}$| . | mas . | |$\mathrm{km\, s^{-1}}$| . |
| Members in Bassino et al. (2000) | |||||
| 314.7366 | –12.6418 | 7.33 ± 0.07 | –15.55 ± 0.05 | 1.41 ± 0.04 | –26.2 ± 0.2a |
| 314.7401 | –12.6294 | 18.41 ± 0.07 | –7.72 ± 0.06 | 2.66 ± 0.05 | –53.1 ± 0.7a |
| 314.7283 | –12.6345 | 2.05 ± 0.09 | –10.80 ± 0.07 | 3.11 ± 0.06 | –8.5 ± 0.6a |
| 314.7222 | –12.6318 | 4.61 ± 0.07 | –7.03 ± 0.05 | 1.52 ± 0.04 | –20.8 ± 0.6a |
| 314.8046 | –12.6706 | –21.38 ± 0.05 | –9.39 ± 0.03 | 1.18 ± 0.03 | |
| 314.7781 | –12.5914 | 3.50 ± 0.05 | –6.02 ± 0.03 | 0.80 ± 0.03 | –11.6 ± 0.1b |
| 314.7776 | –12.5777 | –11.40 ± 0.07 | 1.19 ± 0.05 | 1.91 ± 0.05 | |
| 314.7423 | –12.5768 | –4.60 ± 0.04 | –5.57 ± 0.03 | 0.83 ± 0.03 | |
| 314.7237 | –12.5765 | –4.16 ± 0.04 | –6.62 ± 0.03 | 0.33 ± 0.03 | 51.5 ± 0.1b |
| 314.7378 | –12.5785 | –5.53 ± 0.35 | 2.55 ± 0.23 | 1.78 ± 0.23 | |
| 314.7487 | –12.6955 | 16.82 ± 0.07 | 7.75 ± 0.04 | 1.43 ± 0.04 | –28.2 ± 1.6a |
| α . | δ . | μα cos (δ) . | μδ . | ϖ . | |$v$|r . |
|---|---|---|---|---|---|
| ° . | ° . | |$\mathrm{mas\, yr^{-1}}$| . | |$\mathrm{mas\, yr^{-1}}$| . | mas . | |$\mathrm{km\, s^{-1}}$| . |
| Members in Bassino et al. (2000) | |||||
| 314.7366 | –12.6418 | 7.33 ± 0.07 | –15.55 ± 0.05 | 1.41 ± 0.04 | –26.2 ± 0.2a |
| 314.7401 | –12.6294 | 18.41 ± 0.07 | –7.72 ± 0.06 | 2.66 ± 0.05 | –53.1 ± 0.7a |
| 314.7283 | –12.6345 | 2.05 ± 0.09 | –10.80 ± 0.07 | 3.11 ± 0.06 | –8.5 ± 0.6a |
| 314.7222 | –12.6318 | 4.61 ± 0.07 | –7.03 ± 0.05 | 1.52 ± 0.04 | –20.8 ± 0.6a |
| 314.8046 | –12.6706 | –21.38 ± 0.05 | –9.39 ± 0.03 | 1.18 ± 0.03 | |
| 314.7781 | –12.5914 | 3.50 ± 0.05 | –6.02 ± 0.03 | 0.80 ± 0.03 | –11.6 ± 0.1b |
| 314.7776 | –12.5777 | –11.40 ± 0.07 | 1.19 ± 0.05 | 1.91 ± 0.05 | |
| 314.7423 | –12.5768 | –4.60 ± 0.04 | –5.57 ± 0.03 | 0.83 ± 0.03 | |
| 314.7237 | –12.5765 | –4.16 ± 0.04 | –6.62 ± 0.03 | 0.33 ± 0.03 | 51.5 ± 0.1b |
| 314.7378 | –12.5785 | –5.53 ± 0.35 | 2.55 ± 0.23 | 1.78 ± 0.23 | |
| 314.7487 | –12.6955 | 16.82 ± 0.07 | 7.75 ± 0.04 | 1.43 ± 0.04 | –28.2 ± 1.6a |
a|$v$|r from Gaia DR2.
b|$v$|r from GALAH.
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