HSC 567
0.45
UTI
0.53
CN
0.46
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members)
1.7 [arcmin]
- CN 0.53 Moderately populated
- Cdens 0.46 Loose
- CC3 0.75 High quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
Overview
HSC 567 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a very large* distance, well above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, old cluster (see Parameters). It was recently reported in the literature.
(*): The parallax distance estimate (~10.01 kpc) differs significantly from the median photometric distance (~6.74 kpc).
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Very distant
Moderate extinction
Massive
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 299.026 | 35.986 | 0.1 | -2.906 | -5.054 | -3.469 |
| Hu & Soubiran | 2025 | 299.036 | 35.993 | â | â | â | â |
| Hunt & Reffert | 2024 | 299.022 | 35.985 | 0.093 | -2.916 | -5.036 | â |
| Cavallo et al. | 2024 | 299.036 | 35.993 | 0.092 | â | â | â |
| Hunt & Reffert | 2023 | 299.022 | 35.985 | 0.093 | -2.916 | -5.036 | â |
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 | -0.010* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1073* | â | â |
| Cavallo et al. | 2024 | 4.88 | 1.10 | â | 2138 | -0.080 | â | â | â |
| Hunt & Reffert | 2023 | 8.60 | 2.21 | 1.97 | 443 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.