HSC 766
0.24
UTI
0.26
CN
0.18
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members)
3.0 [arcmin]
- CN 0.26 Poorly populated
- Cdens 0.18 Very loose
- CC3 0.25 Low quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
Overview
HSC 766 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Distant
Moderate extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 329.274 | 52.851 | 0.161 | -3.741 | -3.019 | -39.98 |
| Hu & Soubiran | 2025 | 329.254 | 52.856 | â | â | â | â |
| Hunt & Reffert | 2024 | 329.263 | 52.848 | 0.159 | -3.702 | -3.034 | -40.123 |
| Cavallo et al. | 2024 | 329.254 | 52.856 | 0.16 | â | â | â |
| Hunt & Reffert | 2023 | 329.263 | 52.848 | 0.159 | -3.702 | -3.034 | -40.123 |
đĄ Note: The UCC values are estimated from its identified members.
| Reference | Year | Dist [kpc] | Av [mag] | DAv [mag] | Age [Myr] | [Fe/H] [dex] | Mass [Msun] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.310* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 431* | â | â |
| Cavallo et al. | 2024 | 4.19 | 2.03 | â | 1000 | -0.140 | â | â | â |
| Hunt & Reffert | 2023 | 5.77 | 2.14 | 1.57 | 632 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.