UPK 456
0.12
UTI
0.0
CN
0.24
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
29.1 [arcmin]
- CN 0.0 Sparse
- Cdens 0.24 Very loose
- CC3 0.38 Low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
UPK 456 is a sparse, very loose object of low C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied 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
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 104.828 | -17.137 | 1.981 | -7.651 | 0.14 | 21.197 |
| Cavallo et al. | 2024 | 104.863 | -17.187 | 1.996 | â | â | â |
| Hunt & Reffert | 2023 | 104.822 | -16.772 | 1.994 | -7.75 | 0.18 | 17.166 |
| Sim et al. | 2019 | 104.811 | -17.092 | â | -7.62 | 0.18 | 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 | 0.49 | 0.43 | â | 89 | -0.380 | â | â | â |
| Hunt & Reffert | 2023 | 0.47 | 0.07 | 0.24 | 70 | â | â | â | â |
| Sim et al. | 2019 | 0.51 | â | â | 89 | â | â | â | â |
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.