HSC 1788
Summary
HSC 1788 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.
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 |
|---|---|---|---|---|---|---|
| Hunt & Reffert (2023) | 109.14 | -12.559 | 0.283 | -2.063 | 2.164 | – |
| Cavallo et al. (2024) | 109.16 | -12.507 | 0.286 | – | – | – |
| Hunt & Reffert (2024) | 109.14 | -12.559 | 0.283 | -2.063 | 2.164 | – |
| UCC | 109.133 | -12.507 | 0.29 | -2.069 | 2.152 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=1.413, diffAV50=0.469, MOD50=12.399, logAge50=7.97 |
| Cavallo et al. (2024) | AV50=1.31, dMod50=12.25, logAge50=8.17, [Fe/H]50=0.13 |
| Hunt & Reffert (2024) | MassJ=148.936, MassTot=125.216 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 3811 | 76.0 | 109.13 | -12.44 | 0.29 | -2.09 | 2.15 | 82.3 | 0.04 |
