CWNU 1251
Summary
CWNU 1251 is a poorly populated, very loose object of low C3 quality. It is located at a very close distance from the Sun, below the mid-plane. It was recently reported in the literature.
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. (2022) | 80.006 | -6.971 | 3.744 | -1.465 | -0.107 | – |
| UCC | 79.639 | -6.847 | 3.469 | -0.242 | -0.226 | 14.289 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | A0=0.55, logAge=7.7 |
Search coordinates in Bayestar19