HXWHB 7
Summary
HXWHB 7 is a sparse, very loose object of very low C3 quality. It is located at a relatively close distance from the Sun, near the mid-plane. It is rarely studied in the literature.
This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry.
Warning: contains less than 25 stars with P>0.5 estimated.
Warning: the low UTI value and no obvious signs of duplication (C_dup=0.64) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Hao et al. (2020) | 80.57 | 35.42 | 0.58 | 1.49 | -2.88 | – |
| UCC | 80.64 | 35.32 | 0.55 | 1.542 | -2.872 | 5.901 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hao et al. (2020) | AG=1.18, d_pc=1735.0, logt=7.6 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Gulliver 26 | 36.0 | 80.68 | 35.27 | 0.38 | 1.85 | -2.86 | 14.27 | 0.67 |