CWNU 3273
Summary
CWNU 3273 is a poorly populated, 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 is very likely a unique object, which shares a very small percentage of members with at least one previously reported entry.
Warning: the low UTI value and no obvious signs of duplication (C_dup=0.9) 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. (2023) | 123.687 | -35.69 | 0.246 | -2.952 | 3.201 | – |
| UCC | 123.7 | -35.677 | 0.255 | -2.956 | 3.192 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.35, m-M=12.75, logA=7.1 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| ASCC 45 | 9.7 | 124.09 | -35.66 | 0.25 | -2.86 | 3.23 | – | 0.62 |