FoF 198
(LP 198)
0.49
UTI
0.8
CN
0.45
Cdens
0.75
CC3
0.23
Clit
1.0
Cdup
Nm (P>50%)
246
Core radius and density
3.2 [pc], 2.2 [pc-2]
- CN 0.8 Rich
- Cdens 0.45 Loose
- CC3 0.75 High quality
- Clit 0.23 Rarely studied
- Cdup 1.0 Unique
Overview
FoF 198 is a rich, loose object of high C3 quality. Its parallax locates it at a moderate 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 rarely studied in the literature.
Note: This object contains blue stragglers according to at least one source.
Note: This object shares a large percentage of members with 2 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 | 112.123 | -20.117 | 0.292 | -2.25 | 2.507 | 67.724 |
| Almeida et al. | 2025 | 112.131 | -20.109 | â | â | â | â |
| Hunt & Reffert | 2024 | 112.13 | -20.117 | 0.31 | -2.253 | 2.506 | 67.753 |
| Cavallo et al. | 2024 | 112.133 | -20.12 | 0.308 | â | â | â |
| Hunt & Reffert | 2023 | 112.13 | -20.117 | 0.31 | -2.253 | 2.506 | 67.753 |
| Almeida et al. | 2023 | 112.128 | -20.107 | â | â | â | â |
| Li et al. | 2023 | 112.128 | -20.111 | 0.29 | -2.28 | 2.54 | â |
| Dias et al. | 2021 | 112.131 | -20.109 | 0.265 | -2.262 | 2.505 | â |
| Cantat-Gaudin et al. | 2020 | 112.127 | -20.107 | 0.278 | -2.262 | 2.497 | â |
| Liu & Pang | 2019 | 112.115 | -20.1 | 0.31 | -1.972 | 2.311 | 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 | 2.845 | 1.09 | 2.06 | 276 | -0.160 | 886 | 0.64 | 1 |
| Almeida et al. | 2025 | 2.84 | 1.19 | â | 294 | â | 488 | â | â |
| Hunt & Reffert | 2024 | 2.85 | 0.91 | 2.06 | 173 | â | 886(1) | â | â |
| Cavallo et al. | 2024 | 2.82 | 1.29 | â | 170 | -0.160 | â | â | â |
| Hunt & Reffert | 2023 | 2.85 | 0.91 | 2.06 | 173 | â | â | â | â |
| Almeida et al. | 2023 | 2.84 | 1.18 | â | 276 | -0.127 | 916(1) | 0.64 | â |
| Li et al. | 2023 | 4.17 | 1.00 | â | 631 | 0.097 | â | â | 1(1) |
| Dias et al. | 2021 | 2.84 | 1.19 | â | 294 | -0.176 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.22 | 0.54 | â | 257 | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 537 | -0.750 | 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. Silver sample.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).