HSC 1848
0.06
UTI
0.3
CN
0.14
Cdens
0.12
CC3
0.25
Clit
0.3
Cdup
Stellar density (N50/rad)
0.7 [N/pc2]
- CN 0.3 Poorly populated
- Cdens 0.14 Very loose
- CC3 0.12 Very low quality
- Clit 0.25 Poorly studied
- Cdup 0.3 Possibly duplicate
Overview
HSC 1848 is a poorly populated, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, below 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 age parameter (see Parameters). It was recently reported in the literature.
â ī¸ Warning: This is possibly a duplicate object, which shares a significant 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 | 109.576 | -20.051 | 0.325 | -2.086 | 3.284 | â |
| Liu et al. | 2025 | 109.58 | -20.06 | 0.31 | -2.08 | 3.28 | 66.25 |
| Hunt & Reffert | 2024 | 109.575 | -20.058 | 0.314 | -2.077 | 3.283 | 66.25 |
| Cavallo et al. | 2024 | 109.749 | -19.806 | 0.314 | â | â | â |
| Hunt & Reffert | 2023 | 109.575 | -20.058 | 0.314 | -2.077 | 3.283 | 66.25 |
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 | 2.75 | 0.91 | 2.22 | 245 | -0.320 | 73 | â | â |
| Liu et al. | 2025 | 5.13 | 0.44 | â | 40 | â | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 73(1) | â | â |
| Cavallo et al. | 2024 | 2.31 | 0.93 | â | 245 | -0.320 | â | â | â |
| Hunt & Reffert | 2023 | 2.75 | 0.91 | 2.22 | 257 | 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 primordial binary cluster 211 along with HSC_1847, and of multiple system 61 along with HSC_1847 and UBC_1376.
Palma et al. (2025)
Part of multiple system G133, along with UBC_1376, HSC_1847 and CWNU_2211.
Cavallo et al. (2024)
Gold sample.