CWNU 4888
Summary
CWNU 4888 is a poorly populated, very loose object of intermediate 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) | 274.567 | -32.345 | 0.058 | -3.272 | -6.42 | -0.08 |
| UCC | 274.563 | -32.362 | 0.062 | -3.255 | -6.386 | -0.076 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=0.4, m-M=15.55, logA=9.9 |
Search coordinates in Bayestar19