CWNU 4138
Summary
CWNU 4138 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, well below the mid-plane. It was recently reported in the literature.
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. (2023) | 333.229 | 47.258 | 0.191 | -2.368 | -2.112 | -24.33 |
| UCC | 333.22 | 47.266 | 0.206 | -2.407 | -2.102 | -70.104 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=0.1, m-M=14.15, logA=9.9 |
Search coordinates in Bayestar19