CWNU 1014
Summary
CWNU 1014 is a moderately populated, very dense object of very high C3 quality. It is located at a very close distance from the Sun, near 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, and a small percentage with at least one entry reported in the same catalogue.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2022) | 242.153 | -39.083 | 6.299 | -9.891 | -23.555 | – |
| UCC | 242.201 | -39.07 | 6.276 | -9.91 | -23.433 | -2.536 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | A0=0.35, logAge=6.7 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| OCSN 214 | 85.7 | 242.2 | -39.07 | 6.28 | -9.87 | -23.51 | -2.45 | 0.0 |
| OC 0666 | 43.9 | 242.17 | -39.06 | 6.31 | -10.0 | -23.48 | -2.45 | 0.59 |
| CWNU 1004 | 18.4 | 240.21 | -41.68 | 6.24 | -10.93 | -23.51 | -2.11 | 0.51 |