CWWDL 3607
Summary
CWWDL 3607 is a sparse, very loose object of very 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 is very likely a unique object, which shares a very small percentage of members with at least one previously reported entry, and a very small percentage 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=0.92) 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) | 137.431 | -53.653 | 0.264 | -4.02 | 3.824 | 30.152 |
| UCC | 137.547 | -53.666 | 0.217 | -4.02 | 3.81 | 6.502 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Chi et al. (2023) | logAge=8.12, Z=-0.18 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| FoF 699 | 8.0 | 138.28 | -53.33 | 0.26 | -4.0 | 3.84 | 38.98 | 0.05 |
| CWWDL 197 | 4.0 | 138.16 | -53.39 | 0.24 | -3.98 | 3.79 | 40.49 | 0.03 |