HSC 759
0.28
UTI
0.8
CN
0.23
Cdens
1.0
CC3
0.0
Clit
0.68
Cdup
Stellar density (N50/rad)
1.1 [N/pc2]
- CN 0.8 Rich
- Cdens 0.23 Very loose
- CC3 1.0 Very high quality
- Clit 0.0 Rarely studied
- Cdup 0.68 Likely unique
Overview
HSC 759 is a rich, very loose object of very high C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the absorption parameter (see Parameters). It was recently reported in the literature.
Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 217.139 | 56.046 | 10.088 | -16.242 | -3.025 | -6.114 |
| Zhang et al. | 2024 | 225.147 | 59.386 | â | â | â | â |
| Cavallo et al. | 2024 | 215.891 | 53.702 | 10.19 | â | â | â |
| Hunt & Reffert | 2023 | 225.147 | 59.386 | 10.162 | -16.195 | -3.64 | -7.771 |
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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 0.1 | 0.35 | 0.57 | 160 | 0.088 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | 0.156(1) | â | â | â |
| Cavallo et al. | 2024 | 0.10 | 0.65 | â | 170 | 0.020 | â | â | â |
| Hunt & Reffert | 2023 | 0.10 | 0.05 | 0.57 | 149 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Classified as optical pair P411, along with HSC_1077.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.