HXHWL 44
Summary
HXHWL 44 is a sparse, loose object of low C3 quality. It is located at a relatively close distance from the Sun, above the mid-plane. It is rarely studied in the literature.
This object shares a large percentage of members with a later 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=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) | 39.327 | 62.095 | 0.67 | -0.91 | -0.46 | – |
| UCC | 39.518 | 62.025 | 0.679 | -0.976 | -0.488 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2021) | AG=1.8, m-M=10.8, logAge=7.66, Z=0.017 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Theia 2945 | 96.0 | 39.49 | 62.02 | 0.69 | -1.0 | -0.5 | – | 0.06 |