HSC 1086
0.05
UTI
0.0
CN
0.15
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
8.0 [arcmin]
- CN 0.0 Sparse
- Cdens 0.15 Very loose
- CC3 0.12 Very low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
HSC 1086 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (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.
Relatively close
Moderate extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 34.489 | 60.619 | 0.448 | 1.935 | -1.583 | 17.442 |
| Hu & Soubiran | 2025 | 34.149 | 60.712 | â | â | â | â |
| Cavallo et al. | 2024 | 34.149 | 60.712 | 0.471 | â | â | â |
| Hunt & Reffert | 2023 | 34.668 | 60.583 | 0.471 | 1.919 | -1.587 | -3.13 |
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 | -0.120* | â | â | â |
| Cavallo et al. | 2024 | 1.79 | 2.83 | â | 813 | 0.350 | â | â | â |
| Hunt & Reffert | 2023 | 1.97 | 2.94 | 2.04 | 501 | 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.