HXWHB 8
Summary
HXWHB 8 is a poorly populated, very dense object of intermediate C3 quality. It is located at a relatively close distance from the Sun, near the mid-plane. It is poorly studied in the literature.
Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry, and a moderate percentage with at least one entry reported in the same catalogue.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Hao et al. (2020) | 80.57 | 33.79 | 0.85 | -0.16 | -3.13 | – |
| Hunt & Reffert (2023) | 80.573 | 33.783 | 0.882 | -0.397 | -3.225 | 4.462 |
| Cavallo et al. (2024) | 80.318 | 33.507 | 0.884 | – | – | – |
| UCC | 80.564 | 33.782 | 0.907 | -0.309 | -3.103 | -3.924 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hao et al. (2020) | AG=1.14, d_pc=1178.0, logt=7.24 |
| Hunt & Reffert (2023) | AV50=0.868, diffAV50=1.684, MOD50=10.12, logAge50=7.527 |
| Cavallo et al. (2024) | AV50=1.01, dMod50=10.2, logAge50=7.52, [Fe/H]50=-0.15 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Gulliver 8 | 100.0 | 80.56 | 33.79 | 0.9 | -0.3 | -3.07 | 6.27 | 0.21 |
| Teutsch 89 | 100.0 | 80.56 | 33.77 | 0.9 | -0.35 | -3.12 | -6.34 | 0.46 |
| HXWHB 5 | 31.2 | 80.51 | 33.56 | 0.86 | -0.25 | -3.12 | 51.54 | 0.05 |
