HSC 2032
0.18
UTI
0.26
CN
0.26
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
26.9 [arcmin]
- CN 0.26 Poorly populated
- Cdens 0.26 Loose
- CC3 0.38 Low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
HSC 2032 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young 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
Low extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 99.235 | -44.468 | 1.748 | -6.859 | 8.461 | 25.488 |
| Cavallo et al. | 2024 | 99.531 | -44.511 | 1.726 | â | â | â |
| Hunt & Reffert | 2023 | 99.177 | -44.432 | 1.732 | -6.785 | 8.46 | 24.976 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Cavallo et al. | 2024 | 0.62 | 0.26 | â | 15 | -0.310 | â | â | â |
| Hunt & Reffert | 2023 | 0.56 | 0.08 | 0.35 | 78 | â | â | â | â |
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.