CWNU 1475
Summary
CWNU 1475 is a sparse, moderately dense object of intermediate C3 quality. It is located at a moderate distance from the Sun, near 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) | 182.56 | -62.341 | 0.238 | -6.71 | 1.065 | -1.92 |
| UCC | 182.549 | -62.344 | 0.225 | -6.71 | 1.07 | 49.379 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=3.25, m-M=12.85, logAge=8.3 |
Search coordinates in Bayestar19