CWNU 3290
Summary
CWNU 3290 is a poorly populated, very dense object of high C3 quality. It is located at a large distance from the Sun, above 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) | 90.253 | 32.009 | 0.187 | 0.917 | -1.103 | 10.94 |
| UCC | 90.253 | 32.009 | 0.169 | 0.928 | -1.116 | 10.936 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.4, m-M=13.35, logA=8.4 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HSC 1413 | 90.7 | 90.26 | 32.01 | 0.18 | 0.91 | -1.1 | 10.94 | 0.59 |