CWNU 4615
Summary
CWNU 4615 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, 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: contains less than 25 stars with P>0.5 estimated.
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) | 333.269 | 60.83 | 0.123 | -2.382 | -1.814 | -78.05 |
| UCC | 333.225 | 60.831 | 0.159 | -2.405 | -1.813 | -73.566 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.9, m-M=14.35, logA=8.9 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 4153 | 8.0 | 333.2 | 61.05 | 0.16 | -2.41 | -1.88 | -78.26 | 0.09 |