HSC 2882
0.12
UTI
0.25
CN
0.1
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
208.6 [arcmin]
- CN 0.25 Poorly populated
- Cdens 0.1 Very loose
- CC3 0.25 Low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
HSC 2882 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by low 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.
Very close
Low 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 | 226.649 | -9.786 | 8.772 | -11.205 | -8.395 | -6.326 |
| Cavallo et al. | 2024 | 223.839 | -7.948 | 8.857 | â | â | â |
| Hunt & Reffert | 2023 | 226.701 | -9.775 | 8.911 | -10.628 | -9.075 | -7.657 |
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 | 0.12 | 0.23 | â | 204 | 0.280 | â | â | â |
| Hunt & Reffert | 2023 | 0.11 | 0.07 | 0.32 | 86 | â | â | â | â |
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.