CWNU 492
Summary
CWNU 492 is a moderately populated, very dense object of high C3 quality. It is located at a close distance from the Sun, above the mid-plane. It was recently reported in the literature.
Warning: This is 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. (2022) | 278.655 | -1.851 | 1.15 | -2.2 | -3.07 | – |
| He et al. (2022) | 278.659 | -1.841 | 1.153 | -2.195 | -3.049 | – |
| UCC | 278.68 | -1.858 | 1.124 | -2.198 | -3.058 | -40.736 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | AG=4.3, m-M=9.15, logAge=8.9, Z=0.014 |
| He et al. (2022) | A0=4.1, logAge=6.0 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| OC 0056 | 80.7 | 278.68 | -1.86 | 1.13 | -2.2 | -3.06 | -40.74 | 0.47 |
| UPK 34 | 77.1 | 278.67 | -1.86 | 1.13 | -2.2 | -3.06 | -40.74 | 0.03 |