CWNU 1710
Summary
CWNU 1710 is a sparse, very loose object of high C3 quality. It is located at a moderate distance from the Sun, 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) | 180.45 | -63.889 | 0.341 | -6.701 | 0.84 | -14.04 |
| UCC | 180.461 | -63.883 | 0.338 | -6.702 | 0.848 | 4.345 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.8, m-M=12.45, logAge=7.2 |
Search coordinates in Bayestar19