HSC 1074
0.13
UTI
0.0
CN
0.14
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
21.1 [arcmin]
- CN 0.0 Sparse
- Cdens 0.14 Very loose
- CC3 0.5 Intermediate quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
HSC 1074 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old 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.
Close
Moderate extinction
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 35.603 | 66.548 | 1.133 | 7.66 | 0.839 | -35.736 |
| Hu & Soubiran | 2025 | 35.851 | 66.194 | â | â | â | â |
| Cavallo et al. | 2024 | 35.851 | 66.194 | 1.126 | â | â | â |
| Hunt & Reffert | 2023 | 35.613 | 66.641 | 1.139 | 7.682 | 0.768 | -35.625 |
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 | 0.260* | â | â | â |
| Cavallo et al. | 2024 | 1.00 | 2.77 | â | 1380 | 0.130 | â | â | â |
| Hunt & Reffert | 2023 | 0.86 | 2.50 | 2.33 | 1262 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.