FoF 2094
(LP 2094)
0.78
UTI
0.76
CN
1.0
Cdens
1.0
CC3
0.56
Clit
1.0
Cdup
Stellar density (N50/rad)
26.0 [N/pc2]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.56 Moderately studied
- Cdup 1.0 Unique
Overview
FoF 2094 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near 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 metallicity 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 | 175.483 | -61.96 | 0.571 | -3.693 | 1.308 | -1.862 |
| Li et al. | 2025 | 175.495 | -61.961 | 0.545 | -3.712 | 1.269 | â |
| Hu & Soubiran | 2025 | 175.495 | -61.957 | â | â | â | â |
| Almeida et al. | 2025 | 175.512 | -61.956 | â | â | â | â |
| Hunt & Reffert | 2024 | 175.465 | -61.952 | 0.567 | -3.723 | 1.306 | 18.957 |
| Cavallo et al. | 2024 | 175.495 | -61.957 | 0.573 | â | â | â |
| Hunt & Reffert | 2023 | 175.465 | -61.952 | 0.567 | -3.723 | 1.306 | 18.957 |
| Almeida et al. | 2023 | 175.531 | -61.936 | â | â | â | â |
| Dias et al. | 2021 | 175.512 | -61.956 | 0.544 | -3.697 | 1.269 | â |
| Cantat-Gaudin et al. | 2020 | 175.495 | -61.961 | 0.545 | -3.712 | 1.269 | â |
| Liu & Pang | 2019 | 175.489 | -61.955 | 0.542 | -3.78 | 1.257 | 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 | 1.61 | 0.75 | 0.73 | 246 | -0.016 | 569 | 0.49 | â |
| Li et al. | 2025 | 1.51 | 0.75 | â | 341 | -0.074 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.270(5) | â | â | â |
| Almeida et al. | 2025 | 1.61 | 0.89 | â | 187 | â | 452 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 770(1) | â | â |
| Cavallo et al. | 2024 | 1.43 | 0.65 | â | 617 | -0.210 | â | â | â |
| Hunt & Reffert | 2023 | 1.63 | 0.65 | 0.73 | 309 | â | â | â | â |
| Almeida et al. | 2023 | 1.61 | 0.88 | â | 216 | 0.042 | 569(1) | 0.49 | â |
| Dias et al. | 2021 | 1.61 | 0.89 | â | 187 | 0.121 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.73 | 0.60 | â | 148 | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 275 | 0.250 | 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. Gold sample.
Cavallo et al. (2024)
Gold sample.