HSC 2091
0.46
UTI
0.34
CN
1.0
Cdens
0.75
CC3
0.25
Clit
0.88
Cdup
Stellar density (N50/rad)
7.1 [N/pc2]
- CN 0.34 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.25 Poorly studied
- Cdup 0.88 Very likely unique
Overview
HSC 2091 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Note: This is very likely a unique object, which shares a small 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 | 126.734 | -42.643 | 0.666 | -5.082 | 4.67 | 13.835 |
| Liu et al. | 2025 | 126.74 | -42.66 | 0.66 | -5.06 | 4.63 | 13.82 |
| Hunt & Reffert | 2024 | 126.742 | -42.658 | 0.656 | -5.06 | 4.626 | 13.824 |
| Cavallo et al. | 2024 | 126.743 | -42.646 | 0.656 | â | â | â |
| Hunt & Reffert | 2023 | 126.742 | -42.658 | 0.656 | -5.06 | 4.626 | 13.824 |
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 | 1.53 | 0.71 | 0.66 | 178 | 0.290 | 116 | â | â |
| Liu et al. | 2025 | 2.26 | 0.33 | â | 178 | â | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 116(1) | â | â |
| Cavallo et al. | 2024 | 1.53 | 0.71 | â | 234 | 0.290 | â | â | â |
| Hunt & Reffert | 2023 | 1.43 | 1.02 | 0.66 | 155 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Liu et al. (2025)
Classified as tidal capture (resonant trapping binary) 218 along with Majaess_99, and of multiple system 62 along with Majaess_99 and Theia_1079.
Palma et al. (2025)
Part of multiple system G213, along with OC_0471, CWNU_339, Majaess_99 and Theia_1079.
Cavallo et al. (2024)
Gold sample.