CWNU 4880
Summary
CWNU 4880 is a poorly populated, very loose object of high 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: 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) | 267.641 | -36.554 | 0.072 | -2.408 | -4.678 | – |
| UCC | 267.617 | -36.558 | 0.078 | -2.419 | -4.681 | -73.303 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.2, m-M=15.6, logA=9.1 |
Search coordinates in Bayestar19