FoF 2198
(LP 2198)
0.78
UTI
0.75
CN
1.0
Cdens
0.75
CC3
0.69
Clit
1.0
Cdup
Stellar density (N50/rad)
17.7 [N/pc2]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.69 Moderately studied
- Cdup 1.0 Unique
Overview
FoF 2198 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old 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 | 107.504 | 4.655 | 0.82 | 0.67 | -0.979 | 44.511 |
| Li et al. | 2025 | 107.506 | 4.667 | 0.8 | 0.678 | -1.008 | â |
| Hu & Soubiran | 2025 | 107.519 | 4.664 | â | â | â | â |
| Almeida et al. | 2025 | 107.502 | 4.699 | â | â | â | â |
| Zhang et al. | 2024 | 107.497 | 4.65 | â | â | â | â |
| Hunt & Reffert | 2024 | 107.497 | 4.65 | 0.81 | 0.683 | -0.991 | 42.219 |
| Cavallo et al. | 2024 | 107.519 | 4.664 | 0.818 | â | â | â |
| Hunt & Reffert | 2023 | 107.497 | 4.65 | 0.81 | 0.683 | -0.991 | 42.219 |
| He et al. | 2022 | 107.511 | 4.648 | 0.823 | 0.666 | -0.964 | â |
| Tarricq et al. | 2022 | 107.498 | 4.651 | 0.828 | 0.668 | -0.979 | â |
| Dias et al. | 2021 | 107.502 | 4.699 | 0.801 | 0.669 | -1.017 | 44.391 |
| Cantat-Gaudin et al. | 2020 | 107.506 | 4.667 | 0.8 | 0.678 | -1.008 | â |
| Liu & Pang | 2019 | 107.517 | 4.647 | 0.808 | 0.724 | -1.036 | 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 | 1.19 | 0.81 | 0.91 | 1225 | 0.057 | 306 | â | â |
| Li et al. | 2025 | 1.04 | 0.69 | â | 1673 | -0.163 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | 0.020(5) | â | â | â |
| Almeida et al. | 2025 | 1.19 | 0.81 | â | 1225 | â | 209 | â | â |
| Zhang et al. | 2024 | â | â | â | â | 0.290(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 403(1) | â | â |
| Cavallo et al. | 2024 | 1.25 | 0.84 | â | 955 | 0.300 | â | â | â |
| Hunt & Reffert | 2023 | 1.19 | 0.65 | 0.91 | 822 | â | â | â | â |
| He et al. | 2022 | â | 1.00 | â | 1000 | â | â | â | â |
| Tarricq et al. | 2022 | 1.17 | â | â | 2291 | â | â | â | â |
| Dias et al. | 2021 | 1.19 | 0.81 | â | 1225 | 0.094 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.20 | 0.17 | â | 2042 | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 1590 | -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: intermediate fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.