CWWDL 8417
Summary
CWWDL 8417 is a sparse, very loose object of intermediate C3 quality. It is located at a moderate distance from the Sun, near 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, 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=0.8) 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) | 28.665 | 61.756 | 0.363 | -1.087 | -0.403 | – |
| UCC | 28.643 | 61.781 | 0.345 | -1.117 | -0.389 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Chi et al. (2023) | logAge=8.27, Z=-0.88 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| UBC 414 | 20.0 | 28.48 | 61.98 | 0.32 | -1.03 | -0.28 | – | 0.33 |
| CWWDL 2006 | 8.0 | 28.92 | 61.99 | 0.33 | -1.07 | -0.31 | – | 0.08 |
| HSC 1060 | 4.0 | 29.52 | 61.91 | 0.34 | -1.03 | -0.39 | -15.47 | 0.23 |