CWNU 4751
Summary
CWNU 4751 is a sparse, very loose object of very low C3 quality. It is located at a large distance from the Sun, 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) | 189.517 | -66.593 | 0.182 | -7.341 | -0.108 | -9.69 |
| UCC | 189.559 | -66.59 | 0.161 | -7.365 | -0.112 | 17.129 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.75, m-M=13.6, logA=9.2 |
Search coordinates in Bayestar19