CWNU 4148
Summary
CWNU 4148 is a poorly populated, very loose 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.
Warning: This is possibly a duplicated object, which shares a significant percentage of members with at least one previously reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2023) | 113.028 | -24.702 | 0.137 | -0.775 | 1.425 | 67.6 |
| UCC | 113.026 | -24.7 | 0.137 | -0.772 | 1.409 | 73.597 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.5, m-M=14.15, logA=8.3 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HSC 1914 | 56.1 | 113.04 | -24.71 | 0.14 | -0.77 | 1.39 | 87.43 | 0.2 |