HSC 1785
0.07
UTI
0.0
CN
0.1
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad)
0.5 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.1 Very loose
- CC3 0.25 Low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
đĨ Members
đ Colab
đŦ Bayestar19
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
Overview
HSC 1785 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate 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.
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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 106.141 | -13.715 | 0.315 | -0.588 | -1.255 | â |
| Hu & Soubiran | 2025 | 106.115 | -13.779 | â | â | â | â |
| Cavallo et al. | 2024 | 106.115 | -13.779 | 0.312 | â | â | â |
| Hunt & Reffert | 2023 | 106.154 | -13.71 | 0.312 | -0.608 | -1.245 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 3.07 | 1.47 | 0.96 | 756 | -0.190 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.240(5) | â | â | â |
| Cavallo et al. | 2024 | 2.69 | 1.36 | â | 1122 | -0.140 | â | â | â |
| Hunt & Reffert | 2023 | 3.45 | 1.58 | 0.96 | 389 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.