CWNU 4257
Summary
CWNU 4257 is a sparse, very loose object of high C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It was recently reported in the literature.
Warning: This is possibly a duplicated object, which shares a significant percentage of members with at least one previously reported entry.
Warning: contains less than 25 stars with P>0.5 estimated.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2023) | 99.387 | 13.304 | 0.206 | -0.003 | -0.281 | – |
| UCC | 99.391 | 13.299 | 0.202 | -0.026 | -0.272 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.45, m-M=13.4, logA=7.3 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HSC 1583 | 68.0 | 99.41 | 13.3 | 0.21 | 0.02 | -0.29 | – | 0.26 |