FoF 2059
(LP 2059)
0.64
UTI
0.75
CN
1.0
Cdens
0.75
CC3
0.35
Clit
1.0
Cdup
Stellar density (N50/rad)
5.9 [N/pc2]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.35 Poorly studied
- Cdup 1.0 Unique
Overview
FoF 2059 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by low 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 large percentage of members with 3 later reported entries. 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 | 153.208 | -60.91 | 0.488 | -6.357 | 3.084 | -11.958 |
| Li et al. | 2025 | 153.233 | -60.885 | 0.472 | -6.337 | 3.073 | â |
| Almeida et al. | 2025 | 153.242 | -60.898 | â | â | â | â |
| Almeida et al. | 2023 | 153.26 | -60.902 | â | â | â | â |
| Dias et al. | 2021 | 153.242 | -60.898 | 0.473 | -6.35 | 3.077 | â |
| Cantat-Gaudin et al. | 2020 | 153.233 | -60.885 | 0.472 | -6.337 | 3.073 | â |
| Liu & Pang | 2019 | 153.175 | -60.889 | 0.459 | -6.302 | 3.08 | 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 | 1.89 | 0.59 | â | 226 | -0.006 | 488 | 0.49 | â |
| Li et al. | 2025 | 1.69 | 0.37 | â | 377 | -0.160 | â | â | â |
| Almeida et al. | 2025 | 1.89 | 0.59 | â | 182 | â | 369 | â | â |
| Almeida et al. | 2023 | 2.15 | 0.76 | â | 99 | -0.107 | 607(1) | 0.49 | â |
| Dias et al. | 2021 | 1.89 | 0.59 | â | 182 | 0.095 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.97 | 0.30 | â | 269 | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 562 | 0.500 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit.