CWNU 3870
Summary
CWNU 3870 is a moderately populated, very dense 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.
This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2023) | 267.992 | -24.518 | 0.3 | -0.226 | -0.831 | -4.22 |
| UCC | 267.989 | -24.51 | 0.287 | -0.201 | -0.832 | -29.333 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=6.2, m-M=13.7, logA=9.2 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Ryu 577 | 36.7 | 268.0 | -24.52 | 0.26 | -0.26 | -0.87 | -2.96 | 0.49 |