CWNU 4410
Summary
CWNU 4410 is a sparse, very loose object of intermediate C3 quality. It is located at a large distance from the Sun, 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) | 291.025 | 8.798 | 0.098 | -2.551 | -5.676 | 25.89 |
| UCC | 291.03 | 8.789 | 0.101 | -2.591 | -5.749 | 37.312 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.9, m-M=14.75, logA=9.4 |
Search coordinates in Bayestar19