CWNU 4141
Summary
CWNU 4141 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, near 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) | 250.915 | -45.794 | 0.289 | -3.124 | -4.335 | -76.35 |
| UCC | 250.936 | -45.812 | 0.315 | -3.12 | -4.327 | -32.104 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=7.35, m-M=13.1, logA=6.7 |
Search coordinates in Bayestar19