CWNU 3338
Summary
CWNU 3338 is a sparse, very loose object of high 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) | 107.103 | -28.523 | 0.069 | -0.59 | 1.722 | – |
| UCC | 107.103 | -28.52 | 0.071 | -0.589 | 1.722 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=0.15, m-M=14.5, logA=8.9 |
Search coordinates in Bayestar19