CWNU 1218
Summary
CWNU 1218 is a poorly populated, moderately dense object of high C3 quality. It is located at a close distance from the Sun, below the mid-plane. It was recently reported in the literature.
This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2022) | 96.924 | -9.995 | 1.037 | -3.375 | 0.995 | – |
| UCC | 96.904 | -9.994 | 1.032 | -3.455 | 1.006 | 35.62 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | A0=4.7, logAge=7.15 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| FSR 1140 | 44.0 | 96.82 | -10.1 | 0.99 | -3.45 | 1.03 | 31.25 | 0.35 |