HSC 1776
Summary
HSC 1776 is a sparse, very loose object of intermediate C3 quality. It is located at a moderate distance from the Sun, above 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) | 110.5 | -10.688 | 0.264 | -1.441 | 0.759 | – |
| Cavallo et al. (2024) | 110.515 | -10.698 | 0.264 | – | – | – |
| Hunt & Reffert (2024) | 110.5 | -10.688 | 0.264 | -1.441 | 0.759 | – |
| UCC | 110.535 | -10.694 | 0.259 | -1.454 | 0.745 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.665, diffAV50=0.618, MOD50=12.659, logAge50=8.5 |
| Cavallo et al. (2024) | AV50=0.71, dMod50=12.3, logAge50=8.6, [Fe/H]50=0.02 |
| Hunt & Reffert (2024) | MassJ=179.468, MassTot=124.655 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 3014 | 88.0 | 110.52 | -10.69 | 0.26 | -1.45 | 0.75 | – | 0.02 |