CWNU 4204
Summary
CWNU 4204 is a moderately populated, very dense object of high C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It was recently reported in the literature.
This is very likely a unique object, which shares a very small percentage of members with at least one previously reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2023) | 273.35 | -17.886 | 0.302 | -0.709 | -1.998 | – |
| UCC | 273.351 | -17.892 | 0.32 | -0.698 | -1.999 | 79.883 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=11.9, m-M=12.9, logA=6.3 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| SAI 126 | 8.0 | 273.36 | -17.89 | 0.37 | -0.74 | -2.29 | -17.26 | 0.16 |