FoF 1800
(LP 1800)
0.75
UTI
0.81
CN
1.0
Cdens
0.75
CC3
0.6
Clit
1.0
Cdup
Stellar density (N50/rad)
21.3 [N/pc2]
- CN 0.81 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.6 Moderately studied
- Cdup 1.0 Unique
Overview
FoF 1800 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, 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 | 337.846 | 58.062 | 0.7 | -4.555 | -2.699 | -31.475 |
| Li et al. | 2025 | 337.843 | 58.053 | 0.705 | -4.592 | -2.648 | â |
| Wei et al. | 2025 | 337.809 | 58.056 | 0.705 | -4.554 | -2.71 | â |
| Almeida et al. | 2025 | 337.881 | 58.04 | â | â | â | â |
| Hunt & Reffert | 2024 | 337.824 | 58.045 | 0.698 | -4.55 | -2.706 | -34.687 |
| Cavallo et al. | 2024 | 337.83 | 58.057 | 0.702 | â | â | â |
| Hunt & Reffert | 2023 | 337.824 | 58.045 | 0.698 | -4.55 | -2.706 | -34.687 |
| Almeida et al. | 2023 | 337.898 | 57.989 | â | â | â | â |
| Tarricq et al. | 2022 | 337.792 | 58.036 | 0.707 | -4.558 | -2.715 | â |
| Dias et al. | 2021 | 337.881 | 58.04 | 0.706 | -4.591 | -2.631 | -26.683 |
| Cantat-Gaudin et al. | 2020 | 337.843 | 58.053 | 0.705 | -4.592 | -2.648 | â |
| Liu & Pang | 2019 | 337.809 | 58.069 | 0.709 | -4.571 | -2.633 | 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 | 1.34 | 1.64 | 1.26 | 286 | 0.073 | 955 | 0.465 | â |
| Li et al. | 2025 | 1.17 | 1.36 | â | 377 | 0.054 | â | â | â |
| Wei et al. | 2025 | 1.87 | 1.34 | â | 576 | 0.250 | 893 | 0.45 | â |
| Almeida et al. | 2025 | 1.26 | 1.72 | â | 146 | â | 850 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1065(1) | â | â |
| Cavallo et al. | 2024 | 1.34 | 1.72 | â | 240 | 0.220 | â | â | â |
| Hunt & Reffert | 2023 | 1.35 | 1.56 | 1.26 | 203 | â | â | â | â |
| Almeida et al. | 2023 | 1.33 | 1.76 | â | 189 | 0.038 | 1017(1) | 0.48 | â |
| Tarricq et al. | 2022 | 1.35 | â | â | 355 | â | â | â | â |
| Dias et al. | 2021 | 1.26 | 1.72 | â | 146 | 0.093 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.39 | 1.25 | â | 331 | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 479 | -1.000 | 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.