CWNU 4313
Summary
CWNU 4313 is a sparse, very loose object of low C3 quality. It is located at a 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) | 3.011 | 56.267 | 0.102 | -1.63 | -0.648 | – |
| UCC | 2.99 | 56.265 | 0.112 | -1.63 | -0.668 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.9, m-M=15.25, logA=8.7 |
Search coordinates in Bayestar19