HXHWL 11
Summary
HXHWL 11 is a poorly populated, very loose object of intermediate C3 quality. It is located at a relatively close distance from the Sun, below the mid-plane. It is rarely studied in the literature.
This object shares a small percentage of members with a later reported entry.
Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) 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 |
|---|---|---|---|---|---|---|
| He et al. (2021) | 119.75 | -47.299 | 0.63 | -3.79 | 4.92 | – |
| UCC | 119.946 | -47.256 | 0.633 | -3.808 | 4.928 | 13.141 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2021) | AG=0.9, m-M=11.3, logAge=7.44, Z=0.024 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HSC 2097 | 18.5 | 119.42 | -46.96 | 0.62 | -3.66 | 4.91 | -6.59 | 0.17 |