CWNU 1798
Summary
CWNU 1798 is a poorly populated, dense object of very 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) | 262.849 | -34.014 | 0.383 | 0.076 | -1.055 | – |
| UCC | 262.84 | -34.004 | 0.384 | 0.088 | -1.065 | -39.261 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=5.0, m-M=12.1, logAge=6.4 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Collinder 333 | 93.3 | 262.85 | -34.0 | 0.39 | 0.06 | -1.09 | -23.74 | 0.67 |