UBC 1588
0.53
UTI
0.3
CN
1.0
Cdens
0.75
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad)
5.8 [N/pc2]
- CN 0.3 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.3 Poorly studied
- Cdup 1.0 Unique
Overview
UBC 1588 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 183.681 | -60.325 | 0.244 | -6.851 | 0.732 | -30.712 |
| Hunt & Reffert | 2024 | 183.685 | -60.324 | 0.261 | -6.851 | 0.725 | -30.781 |
| Cavallo et al. | 2024 | 183.718 | -60.331 | 0.257 | â | â | â |
| Hunt & Reffert | 2023 | 183.685 | -60.324 | 0.261 | -6.851 | 0.725 | -30.781 |
| Castro-Ginard et al. | 2022 | 183.71 | -60.33 | 0.25 | -6.86 | 0.73 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 3.775 | 1.435 | 2.03 | 13 | 0.770 | 455 | â | â |
| Liu et al. | 2025 | 6.17 | 0.69 | â | 13 | â | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 455(1) | â | â |
| Cavallo et al. | 2024 | 3.05 | 1.04 | â | 145 | 0.770 | â | â | â |
| Hunt & Reffert | 2023 | 3.72 | 1.94 | 2.03 | 13 | â | â | â | â |
| Castro-Ginard et al. | 2022 | 3.83 | 1.83 | â | 8 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Liu et al. (2025)
Classified as primordial binary cluster 117 along with CWNU_2634.
Palma et al. (2025)
Classified as optical pair (not dynamically associated) P204, along with CWNU_2634.
Cavallo et al. (2024)
Silver sample.