HSC 1032
0.02
UTI
0.0
CN
0.08
Cdens
0.0
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
13.4 [arcmin]
- CN 0.0 Sparse
- Cdens 0.08 Very loose
- CC3 0.0 Very low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
HSC 1032 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as an 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.
Relatively close
Moderate extinction
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 24.657 | 60.922 | 0.533 | 1.669 | -3.279 | -31.299 |
| Hunt & Reffert | 2023 | 24.497 | 60.961 | 0.534 | 1.661 | -3.305 | -8.49 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2023 | 1.74 | 1.10 | 1.13 | 3707 | â | â | â | â |
Hunt & Reffert (2024)
Classified as a moving group.