CWNU 1070
Summary
CWNU 1070 is a poorly populated, loose object of high C3 quality. It is located at a relatively close distance from the Sun, above the mid-plane. It was recently reported in the literature.
This object shares a moderate percentage of members with at least one entry reported in the same catalogue.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2022) | 52.658 | 59.843 | 0.902 | -1.939 | -0.734 | – |
| UCC | 52.677 | 59.818 | 0.898 | -1.958 | -0.747 | -27.482 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | A0=1.85, logAge=7.15 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Theia 1722 | 100.0 | 52.68 | 59.96 | 0.9 | -1.96 | -0.7 | -18.92 | 0.29 |
| CWWDL 14458 | 57.6 | 52.54 | 59.8 | 0.89 | -2.01 | -0.75 | -10.74 | 0.05 |
| CWNU 1058 | 36.4 | 51.4 | 60.1 | 0.89 | -2.06 | -0.73 | -9.57 | 0.35 |