CWNU 4891
Summary
CWNU 4891 is a sparse, very loose object of very low C3 quality. It is located at a large distance from the Sun, above 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) | 273.307 | -5.933 | 0.2 | -2.151 | -4.462 | – |
| UCC | 273.283 | -5.961 | 0.191 | -2.129 | -4.395 | -12.079 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=3.05, m-M=14.65, logA=9.6 |
Search coordinates in Bayestar19