CWWDL 14193
Summary
CWWDL 14193 is a sparse, very loose object of high 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) | 253.422 | -41.491 | 0.662 | -0.648 | -1.937 | -30.8 |
| UCC | 253.36 | -41.474 | 0.632 | -0.662 | -1.937 | -15.256 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Chi et al. (2023) | logAge=6.28, Z=-0.88 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| NGC 6231 | 16.0 | 253.56 | -41.83 | 0.6 | -0.58 | -2.18 | -27.67 | 1.0 |
| UBC 672 | 4.0 | 253.28 | -41.61 | 0.57 | -0.64 | -2.02 | -26.66 | 0.1 |