CWNU 4312
Summary
CWNU 4312 is a sparse, very loose object of low C3 quality. It is located at a very large 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) | 146.786 | -61.573 | 0.074 | -3.159 | 2.562 | 114.5 |
| UCC | 146.784 | -61.567 | 0.072 | -3.177 | 2.559 | 91.805 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=0.4, m-M=14.95, logA=9.5 |
Search coordinates in Bayestar19