CWWDL 2501
Summary
CWWDL 2501 is a sparse, very loose object of very low C3 quality. It is located at a relatively close distance from the Sun, above the mid-plane. It was recently reported in the literature.
This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry.
Warning: contains less than 25 stars with P>0.5 estimated.
Warning: the low UTI value and no obvious signs of duplication (C_dup=0.84) 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) | 305.429 | 38.781 | 0.564 | -3.28 | -5.691 | -3.113 |
| UCC | 305.475 | 38.742 | 0.561 | -3.283 | -5.684 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Chi et al. (2023) | logAge=6.2, Z=0.4 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| FoF 2179 | 16.0 | 305.39 | 38.61 | 0.56 | -3.25 | -5.98 | -22.57 | 0.58 |
| Collinder 422 | 12.0 | 305.93 | 38.5 | 0.56 | -3.42 | -5.79 | -21.9 | 0.95 |
| UBC 140 | 12.0 | 305.37 | 38.6 | 0.56 | -3.24 | -6.0 | -22.57 | 0.14 |
| Berkeley 86 | 4.0 | 305.08 | 38.71 | 0.56 | -3.44 | -5.43 | -0.48 | 0.9 |
| OC 0114 | 4.0 | 305.81 | 38.94 | 0.57 | -3.42 | -5.73 | 5.16 | 0.13 |