CWWDL 8449
Summary
CWWDL 8449 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It was recently reported in the literature.
This object shares a very small percentage of members with a later 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=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 |
|---|---|---|---|---|---|---|
| Chi et al. (2023) | 29.892 | 62.066 | 0.314 | -0.993 | -0.21 | -58.83 |
| UCC | 29.763 | 62.034 | 0.336 | -1.014 | -0.22 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Chi et al. (2023) | logAge=6.8, Z=0.42 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HSC 1060 | 4.0 | 29.52 | 61.91 | 0.34 | -1.03 | -0.39 | -15.47 | 0.23 |