CWNU 48
Summary
CWNU 48 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.
This is likely a unique object, which shares a moderate 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. (2022) | 100.293 | -23.789 | 0.96 | -1.34 | 2.34 | – |
| UCC | 100.27 | -23.829 | 0.975 | -1.392 | 2.393 | 30.355 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | AG=1.35, m-M=10.7, logAge=7.4, Z=0.002 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HXHWL 69 | 32.0 | 101.15 | -24.3 | 0.96 | -1.52 | 2.46 | 36.01 | 0.47 |
| Theia 3740 | 24.0 | 101.17 | -24.29 | 0.96 | -1.52 | 2.46 | 36.4 | 0.01 |