CWNU 4879
Summary
CWNU 4879 is a sparse, very loose object of intermediate C3 quality. It is located at a very large distance from the Sun, well 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) | 256.894 | -32.438 | 0.094 | -3.143 | -5.473 | 9.43 |
| UCC | 256.896 | -32.423 | 0.093 | -3.243 | -5.45 | 15.189 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.3, m-M=15.5, logA=9.8 |
Search coordinates in Bayestar19