CWNU 3587
Summary
CWNU 3587 is a sparse, moderately dense object of low 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 likely a duplicate object, which shares a large 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) | 333.177 | 58.282 | 0.216 | -4.654 | -2.252 | -70.7 |
| UCC | 333.135 | 58.292 | 0.206 | -4.645 | -2.241 | -70.703 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=3.7, m-M=12.95, logA=8.8 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HSC 806 | 76.0 | 333.13 | 58.28 | 0.21 | -4.59 | -2.24 | -70.78 | 0.26 |