CWNU 3298
Summary
CWNU 3298 is a rich, very dense object of high C3 quality. It is located at a large distance from the Sun, below the mid-plane. It was recently reported in the literature.
This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2023) | 146.73 | -56.143 | 0.177 | -5.392 | 4.191 | 40.02 |
| UCC | 146.729 | -56.141 | 0.179 | -5.402 | 4.191 | 39.096 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=3.6, m-M=13.4, logA=8.2 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HSC 2274 | 49.0 | 146.73 | -56.14 | 0.16 | -5.4 | 4.21 | 40.94 | 0.52 |