UBC 1222
0.52
UTI
0.61
CN
0.63
Cdens
0.75
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members)
4.4 [arcmin]
- CN 0.61 Moderately populated
- Cdens 0.63 Moderately dense
- CC3 0.75 High quality
- Clit 0.31 Poorly studied
- Cdup 1.0 Unique
Overview
UBC 1222 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.
Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.
Distant
Moderate 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 | 24.519 | 56.508 | 0.268 | -1.347 | -0.639 | â |
| Zhang et al. | 2024 | 24.508 | 56.508 | â | â | â | â |
| Hunt & Reffert | 2024 | 24.508 | 56.508 | 0.28 | -1.348 | -0.645 | â |
| Cavallo et al. | 2024 | 24.514 | 56.503 | 0.28 | â | â | â |
| Hunt & Reffert | 2023 | 24.508 | 56.508 | 0.28 | -1.348 | -0.645 | â |
| Castro-Ginard et al. | 2022 | 24.52 | 56.5 | 0.29 | -1.35 | -0.63 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Zhang et al. | 2024 | â | â | â | â | -0.221* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 535* | â | â |
| Cavallo et al. | 2024 | 3.30 | 1.79 | â | 29 | -0.150 | â | â | â |
| Hunt & Reffert | 2023 | 3.30 | 1.44 | 2.03 | 199 | â | â | â | â |
| Castro-Ginard et al. | 2022 | 3.55 | 1.12 | â | 132 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.