CWNU 2030
Summary
CWNU 2030 is a sparse, very loose object of very low C3 quality. It is located at a moderate 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) | 329.583 | 45.148 | 0.253 | -3.243 | -3.636 | -18.15 |
| UCC | 329.592 | 45.094 | 0.246 | -3.257 | -3.664 | -18.146 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=0.45, m-M=12.9, logAge=9.7 |
Search coordinates in Bayestar19