CWNU 4814
Summary
CWNU 4814 is a poorly populated, very loose object of intermediate C3 quality. It is located at a large distance from the Sun, well above 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. (2023) | 267.388 | -17.684 | 0.097 | -3.376 | -5.92 | – |
| UCC | 267.385 | -17.696 | 0.11 | -3.344 | -5.899 | 101.477 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.5, m-M=15.85, logA=9.6 |
Search coordinates in Bayestar19