FoF 2220
(LP 2220)
0.75
UTI
0.75
CN
1.0
Cdens
0.75
CC3
0.62
Clit
1.0
Cdup
Stellar density (N50/rad)
7.9 [N/pc2]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.62 Moderately studied
- Cdup 1.0 Unique
Overview
FoF 2220 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 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 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 | 127.442 | -41.334 | 0.735 | -1.77 | 1.108 | -6.236 |
| Li et al. | 2025 | 127.45 | -41.343 | 0.716 | -1.762 | 1.07 | â |
| Hu & Soubiran | 2025 | 127.442 | -41.294 | â | â | â | â |
| Almeida et al. | 2025 | 127.458 | -41.343 | â | â | â | â |
| Hunt & Reffert | 2024 | 127.411 | -41.272 | 0.732 | -1.774 | 1.126 | 0.882 |
| Cavallo et al. | 2024 | 127.442 | -41.294 | 0.736 | â | â | â |
| Hunt & Reffert | 2023 | 127.411 | -41.272 | 0.732 | -1.774 | 1.126 | 0.882 |
| Almeida et al. | 2023 | 127.447 | -41.365 | â | â | â | â |
| Tarricq et al. | 2022 | 127.437 | -41.331 | 0.732 | -1.776 | 1.111 | â |
| Dias et al. | 2021 | 127.458 | -41.343 | 0.718 | -1.768 | 1.093 | 2.699 |
| Cantat-Gaudin et al. | 2020 | 127.45 | -41.343 | 0.716 | -1.762 | 1.07 | â |
| Liu & Pang | 2019 | 127.472 | -41.33 | 0.719 | -1.759 | 1.134 | 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 | 1.29 | 0.89 | 1.17 | 597 | -0.175 | 351 | 0.42 | â |
| Li et al. | 2025 | 1.19 | 0.89 | â | 716 | -0.250 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.250(5) | â | â | â |
| Almeida et al. | 2025 | 1.29 | 1.00 | â | 597 | â | 243 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 351(1) | â | â |
| Cavallo et al. | 2024 | 1.30 | 0.50 | â | 1349 | 0.280 | â | â | â |
| Hunt & Reffert | 2023 | 1.28 | 0.66 | 1.17 | 540 | â | â | â | â |
| Almeida et al. | 2023 | 1.29 | 1.06 | â | 507 | -0.100 | 365(1) | 0.42 | â |
| Tarricq et al. | 2022 | 1.31 | â | â | 490 | â | â | â | â |
| Dias et al. | 2021 | 1.29 | 1.00 | â | 597 | -0.075 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.35 | 0.68 | â | 457 | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 1150 | -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. Gold sample.
Cavallo et al. (2024)
Gold sample.