CWWDL 4776
Summary
CWWDL 4776 is a poorly populated, very loose object of low C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It was recently reported in the literature.This is a unique object, which shares a very small percentage of members with at least one previously reported entry.
Warning: the low UTI value and no obvious signs of duplication (C_dup=0.96) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Chi et al. (2023) | 116.502 | -26.629 | 0.324 | -2.177 | 2.536 | – |
| UCC | 116.509 | -26.629 | 0.31 | -2.198 | 2.557 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Chi et al. (2023) | logAge=7.7, Z=0.4 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 3133 | 3.7 | 116.49 | -26.7 | 0.33 | -2.08 | 2.28 | 53.55 | 0.04 |
| HSC 1946 | 3.7 | 116.48 | -26.7 | 0.33 | -2.08 | 2.27 | 53.55 | 0.25 |
| UBC 1394 | 3.7 | 116.46 | -26.6 | 0.29 | -2.24 | 2.81 | – | 0.39 |