CWNU 1935
Summary
CWNU 1935 is a sparse, very loose object of low C3 quality. It is located at a relatively close 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) | 63.582 | 44.817 | 0.701 | 1.258 | -1.26 | – |
| UCC | 63.574 | 44.826 | 0.689 | 1.228 | -1.262 | -2.714 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.75, m-M=10.6, logAge=8.7 |
Search coordinates in Bayestar19