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Table 2.
Additional likely members selected for visible spectroscopy.
| Star | π | μα cos δ | μδ | RUWE | GBP | GRP | SVKY (1) | KGF (2) |
|---|---|---|---|---|---|---|---|---|
| (mas) | (mas yr1) | (mas yr1) | nr. | nr. | ||||
| 183114.83−020350.0 | 1.5419 ± 0.1177 | −0.177 ± 0.115 | −8.211 ± 0.105 | 4.980 | 14.099 ± 0.004 | 10.799 ± 0.005 | 5 | 36 |
| 183119.37−021229.5 | 1.9350 ± 0.0953 | −0.691 ± 0.074 | −6.981 ± 0.062 | 3.153 | 13.467 ± 0.003 | 10.601 ± 0.004 | ||
| 183123.97−020529.5 | 1.7822 ± 0.0953 | +0.317 ± 0.096 | −6.347 ± 0.090 | 2.358 | 16.077 ± 0.007 | 12.039 ± 0.007 | 2A | 99 |
| 183126.02−020517.0 | 2.0323 ± 0.3693 | −1.815 ± 0.401 | −7.683 ± 0.342 | 3.699 | 19.846 ± 0.057 | 14.879 ± 0.019 | 1C | 122 |
| 183127.81−020521.8 | 2.1396 ± 0.1025 | −0.616 ± 0.112 | −10.035 ± 0.096 | 0.977 | 1A-N | |||
| 183127.83−020523.7 | 2.4575 ± 0.2611 | −0.035 ± 0.285 | −7.830 ± 0.243 | 6.319 | 14.792 ± 0.006 | 10.839 ± 0.007 | 1A-S | 141 |
| 183129.61−020833.8 | 2.0220 ± 0.1171 | +0.264 ± 0.112 | −9.363 ± 0.103 | 1.387 | 18.508 ± 0.024 | 13.982 ± 0.004 | ||
| 183132.18−021531.2 | 1.9776 ± 0.0835 | −1.092 ± 0.066 | −9.858 ± 0.057 | 0.991 | 18.476 ± 0.019 | 15.498 ± 0.007 | ||
| 183144.27−021621.2 | 3.5802 ± 0.7898 | +0.325 ± 0.680 | −4.275 ± 0.638 | 2.474 | 21.790 ± 0.493 | 16.935 ± 0.051 |
Notes. (1) SVKY: Source identifyer in Shuping et al. (2012). (2) KGF: Source identifyer in Kuhn et al. (2010).
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