CWNU 1853
Summary
CWNU 1853 is a poorly 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.
Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2023) | 275.75 | -14.648 | 0.343 | -0.801 | -2.508 | – |
| UCC | 275.752 | -14.653 | 0.347 | -0.793 | -2.503 | -25.526 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.75, m-M=12.6, logAge=6.25 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Kharchenko 3 | 97.1 | 275.76 | -14.64 | 0.35 | -0.8 | -2.5 | -14.71 | 0.52 |