CWNU 4617
Summary
CWNU 4617 is a sparse, very loose object of very low C3 quality. It is located at a very 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) | 325.098 | 55.561 | 0.071 | -2.419 | -2.06 | – |
| UCC | 325.08 | 55.561 | 0.07 | -2.418 | -2.055 | -105.895 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=6.05, m-M=17.4, logA=6.6 |
Search coordinates in Bayestar19