CWNU 1948
Summary
CWNU 1948 is a sparse, very loose object of low 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) | 256.362 | -27.929 | 0.404 | -0.755 | -3.018 | – |
| UCC | 256.31 | -27.885 | 0.386 | -0.749 | -3.032 | -51.014 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.0, m-M=12.5, logAge=9.25 |
Search coordinates in Bayestar19