CWNU 1764
Summary
CWNU 1764 is a sparse, moderately dense object of low C3 quality. It is located at a relatively close 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) | 152.049 | -56.308 | 0.625 | -7.735 | 3.946 | 0.19 |
| UCC | 152.057 | -56.318 | 0.623 | -7.735 | 3.967 | -0.884 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=0.5, m-M=11.15, logAge=6.9 |
Search coordinates in Bayestar19