CWNU 4175
Summary
CWNU 4175 is a moderately 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 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) | 354.603 | 68.525 | 0.948 | -2.405 | -2.942 | -3.3 |
| UCC | 354.571 | 68.496 | 0.948 | -2.393 | -2.939 | -11.413 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.55, m-M=10.05, logA=7.1 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HSC 925 | 42.4 | 354.77 | 68.54 | 0.95 | -2.38 | -2.92 | -6.44 | 0.29 |