UBC 563
0.76
UTI
0.61
CN
1.0
Cdens
1.0
CC3
0.6
Clit
1.0
Cdup
Stellar density (N50/rad)
21.4 [N/pc2]
- CN 0.61 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.6 Moderately studied
- Cdup 1.0 Unique
Overview
UBC 563 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above 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 moderately studied in the literature.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 256.744 | -30.704 | 0.887 | -0.534 | -4.168 | -14.658 |
| Li et al. | 2025 | 256.749 | -30.673 | 0.891 | -0.528 | -4.161 | â |
| Almeida et al. | 2025 | 256.746 | -30.704 | â | â | â | â |
| Hunt & Reffert | 2024 | 256.746 | -30.687 | 0.885 | -0.524 | -4.19 | -10.9 |
| Cavallo et al. | 2024 | 256.739 | -30.722 | 0.888 | â | â | â |
| Hunt & Reffert | 2023 | 256.746 | -30.687 | 0.885 | -0.524 | -4.19 | -10.9 |
| Almeida et al. | 2023 | 256.741 | -30.702 | â | â | â | â |
| He et al. | 2022 | 256.751 | -30.683 | 0.885 | -0.519 | -4.168 | â |
| Dias et al. | 2021 | 256.746 | -30.704 | 0.88 | -0.529 | -4.184 | â |
| Cantat-Gaudin et al. | 2020 | 256.749 | -30.673 | 0.891 | -0.528 | -4.161 | â |
| Castro-Ginard et al. | 2020 | 256.767 | -30.688 | 0.891 | -0.53 | -4.181 | 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 | 1.06 | 1.775 | 1.71 | 209 | 0.059 | 129 | 0.48 | â |
| Li et al. | 2025 | 0.90 | 1.61 | â | 546 | -0.142 | â | â | â |
| Almeida et al. | 2025 | 1.11 | 1.66 | â | 400 | â | 121 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 407(1) | â | â |
| Cavallo et al. | 2024 | 1.05 | 1.94 | â | 309 | 0.010 | â | â | â |
| Hunt & Reffert | 2023 | 1.06 | 1.89 | 1.71 | 134 | â | â | â | â |
| Almeida et al. | 2023 | 1.06 | 1.90 | â | 145 | 0.107 | 129(1) | 0.48 | â |
| He et al. | 2022 | â | 2.10 | â | 112 | â | â | â | â |
| Tarricq et al. | 2022 | 1.05 | â | â | 209 | â | â | â | â |
| Dias et al. | 2021 | 1.11 | 1.66 | â | 400 | 0.125 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.08 | 1.23 | â | 191 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.
Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit. Silver sample.