CWWDL 3813
Summary
CWWDL 3813 is a poorly populated, very loose object of low C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It was recently reported in the literature.
This object shares a large percentage of members with 3 later reported entries.
Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) 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) | 109.538 | -20.05 | 0.311 | -1.999 | 3.312 | – |
| UCC | 109.575 | -20.05 | 0.319 | -2.024 | 3.312 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Chi et al. (2023) | logAge=5.85, Z=0.44 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HSC 1848 | 77.8 | 109.58 | -20.05 | 0.32 | -2.09 | 3.28 | – | 0.06 |
| CWNU 3952 | 14.8 | 109.5 | -19.99 | 0.31 | -1.69 | 3.34 | – | 0.02 |
| HSC 1847 | 11.1 | 109.5 | -20.01 | 0.32 | -1.69 | 3.35 | – | 0.17 |