CWNU 4299
Summary
CWNU 4299 is a sparse, very loose object of high C3 quality. It is located at a moderate 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) | 74.611 | 45.682 | 0.196 | 0.219 | -0.641 | – |
| UCC | 74.611 | 45.68 | 0.206 | 0.225 | -0.641 | -8.813 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.6, m-M=13.05, logA=7.4 |
Search coordinates in Bayestar19