CWNU 3250
Summary
CWNU 3250 is a sparse, very 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 very 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) | 306.687 | 46.82 | 0.364 | -2.027 | -4.7 | -8.61 |
| UCC | 306.687 | 46.82 | 0.377 | -2.009 | -4.708 | -8.613 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=3.0, m-M=11.9, logA=7.8 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HSC 657 | 92.0 | 306.69 | 46.81 | 0.38 | -2.03 | -4.72 | -22.16 | 0.39 |