UBC 1522
0.02
UTI
0.66
CN
1.0
Cdens
0.75
CC3
0.31
Clit
0.02
Cdup
Radius (P>50% members)
3.7 [arcmin]
- CN 0.66 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.31 Poorly studied
- Cdup 0.02 Very likely duplicate
Overview
UBC 1522 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
â ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.
Relatively close
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 | 198.223 | -64.264 | 0.46 | -4.347 | -0.531 | -18.401 |
| Hu & Soubiran | 2025 | 198.204 | -64.259 | â | â | â | â |
| Hunt & Reffert | 2024 | 198.237 | -64.276 | 0.461 | -4.35 | -0.541 | -23.455 |
| Cavallo et al. | 2024 | 198.204 | -64.259 | 0.461 | â | â | â |
| Hunt & Reffert | 2023 | 198.237 | -64.276 | 0.461 | -4.35 | -0.541 | -23.455 |
| Castro-Ginard et al. | 2022 | 198.19 | -64.26 | 0.45 | -4.34 | -0.52 | -17.69 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.120* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 659* | â | â |
| Cavallo et al. | 2024 | 1.79 | 1.66 | â | 759 | 0.010 | â | â | â |
| Hunt & Reffert | 2023 | 2.02 | 1.46 | 1.09 | 670 | â | â | â | â |
| Castro-Ginard et al. | 2022 | 2.58 | 1.03 | â | 778 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.