UBC 51
0.78
UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
10.3 [arcmin]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
UBC 51 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is moderately studied in the literature.
Relatively close
Moderate extinction
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 59.648 | 52.523 | 0.91 | -0.28 | -1.318 | -10.009 |
| Li et al. | 2025 | 59.648 | 52.56 | 0.879 | -0.279 | -1.275 | â |
| Almeida et al. | 2025 | 59.689 | 52.55 | â | â | â | â |
| Zhang et al. | 2024 | 59.769 | 52.642 | â | â | â | â |
| Hunt & Reffert | 2024 | 59.769 | 52.642 | 0.926 | -0.258 | -1.354 | -8.154 |
| Celli et al. | 2024 | 59.668 | 52.559 | â | â | â | â |
| Cavallo et al. | 2024 | 59.614 | 52.509 | 0.92 | â | â | â |
| Hunt & Reffert | 2023 | 59.769 | 52.642 | 0.926 | -0.258 | -1.354 | -8.154 |
| He et al. | 2022 | 59.575 | 52.495 | 0.919 | -0.28 | -1.328 | â |
| Dias et al. | 2021 | 59.689 | 52.55 | 0.863 | -0.268 | -1.312 | â |
| Cantat-Gaudin et al. | 2020 | 59.648 | 52.56 | 0.879 | -0.279 | -1.275 | â |
| Cantat-Gaudin & Anders | 2020 | 59.648 | 52.56 | 0.879 | -0.279 | -1.275 | â |
| Castro-Ginard et al. | 2019 | 59.668 | 52.559 | 0.881 | -0.232 | -1.366 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 0.96 | 1.19 | â | 12 | -0.339 | â | â | â |
| Almeida et al. | 2025 | 1.11 | 1.39 | â | 10 | â | 211 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.191* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 334* | â | â |
| Celli et al. | 2024 | â | â | â | 10 | â | 193 | â | â |
| Cavallo et al. | 2024 | 1.05 | 1.40 | â | 5 | -0.200 | â | â | â |
| Hunt & Reffert | 2023 | 1.04 | 1.24 | 1.76 | 6 | â | â | â | â |
| He et al. | 2022 | â | 1.85 | â | 8 | â | â | â | â |
| Dias et al. | 2021 | 1.11 | 1.39 | â | 10 | -0.109 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.05 | 0.79 | â | 10 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.10 | â | â | â | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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