HSC 2114
0.07
UTI
0.0
CN
0.11
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
11.6 [arcmin]
- CN 0.0 Sparse
- Cdens 0.11 Very loose
- CC3 0.25 Low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
HSC 2114 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.
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
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 127.352 | -45.262 | 0.569 | -6.033 | 4.61 | â |
| Cavallo et al. | 2024 | 127.564 | -45.289 | 0.569 | â | â | â |
| Hunt & Reffert | 2023 | 127.176 | -45.314 | 0.566 | -6.065 | 4.564 | â |
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 | 1.80 | 1.52 | â | 68 | 0.340 | â | â | â |
| Hunt & Reffert | 2023 | 1.68 | 1.81 | 1.12 | 86 | â | â | â | â |
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.