CWNU 4177
Summary
CWNU 4177 is a sparse, very loose object of low 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: 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) | 267.852 | -35.463 | 0.104 | -2.375 | -4.319 | -97.07 |
| UCC | 267.805 | -35.464 | 0.095 | -2.365 | -4.312 | -42.325 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.2, m-M=15.65, logA=9.4 |
Search coordinates in Bayestar19