CWNU 4132
Summary
CWNU 4132 is a sparse, very dense object of intermediate C3 quality. It is located at a moderate distance from the Sun, near 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) | 112.75 | -18.916 | 0.262 | -1.999 | 2.358 | – |
| UCC | 112.75 | -18.93 | 0.269 | -1.988 | 2.357 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.75, m-M=12.8, logA=7.0 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HSC 1853 | 92.0 | 112.75 | -18.93 | 0.26 | -1.99 | 2.35 | – | 0.48 |