CWNU 4777
Summary
CWNU 4777 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It was recently reported in the literature.
Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry.
Warning: contains less than 25 stars with P>0.5 estimated.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2023) | 87.362 | 27.66 | 0.21 | 0.496 | -0.032 | 25.27 |
| UCC | 87.361 | 27.7 | 0.213 | 0.492 | -0.031 | 25.271 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.4, m-M=13.15, logA=9.0 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HSC 1431 | 76.0 | 87.36 | 27.62 | 0.2 | 0.51 | -0.06 | 25.27 | 0.07 |