CWNU 3837
Summary
CWNU 3837 is a poorly populated, very loose object of low C3 quality. It is located at a large distance from the Sun, well above the mid-plane. It was recently reported in the literature.
This object shares a very small percentage of members with at least one entry reported in the same catalogue.
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 |
|---|---|---|---|---|---|---|
| He et al. (2023) | 320.261 | 57.252 | 0.129 | -2.448 | -2.235 | -83.58 |
| UCC | 320.278 | 57.256 | 0.136 | -2.476 | -2.254 | -82.981 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=3.25, m-M=13.6, logA=8.9 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 3895 | 5.9 | 320.71 | 57.13 | 0.13 | -2.38 | -2.09 | -98.29 | 0.05 |