CWNU 2499
Summary
CWNU 2499 is a poorly populated, loose object of low C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It was recently reported in the literature.
This object shares a large percentage of members with a later reported entry.
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. (2023) | 5.42 | 63.054 | 0.229 | -1.808 | -0.606 | – |
| UCC | 5.421 | 63.055 | 0.222 | -1.813 | -0.606 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=4.0, m-M=13.45, logAge=6.6 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Teutsch J0021.7+6303 | 97.2 | 5.42 | 63.06 | 0.22 | -1.82 | -0.61 | -128.6 | 0.02 |