CWNU 103
Summary
CWNU 103 is a sparse, loose object of 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 object shares a moderate percentage of members 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=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 |
|---|---|---|---|---|---|---|
| He et al. (2022) | 30.775 | 68.449 | 0.98 | 0.78 | 0.58 | – |
| UCC | 30.683 | 68.445 | 0.984 | 0.754 | 0.574 | -18.336 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | AG=1.4, m-M=10.8, logAge=6.2, Z=0.002 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Theia 4940 | 52.0 | 30.07 | 68.61 | 0.99 | 0.74 | 0.59 | -23.86 | 0.09 |
| CWNU 377 | 36.0 | 29.99 | 68.64 | 0.99 | 0.65 | 0.62 | -34.08 | 0.15 |