FoF 2000
(LP 2000)
0.65
UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members)
7.3 [arcmin]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.38 Poorly studied
- Cdup 1.0 Unique
Overview
FoF 2000 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 moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.
Relatively close
Moderate extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 319.089 | 57.462 | 0.714 | -3.093 | -4.475 | -21.357 |
| Almeida et al. | 2025 | 319.079 | 57.455 | â | â | â | â |
| Almeida et al. | 2023 | 319.049 | 57.478 | â | â | â | â |
| Tarricq et al. | 2022 | 319.126 | 57.474 | 0.704 | -3.11 | -4.487 | â |
| Dias et al. | 2021 | 319.079 | 57.455 | 0.714 | -3.113 | -4.449 | â |
| Cantat-Gaudin et al. | 2020 | 319.099 | 57.463 | 0.71 | -3.102 | -4.407 | â |
| Liu & Pang | 2019 | 319.038 | 57.459 | 0.701 | -3.1 | -4.402 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 1.27 | 1.66 | â | 154 | â | 413 | â | â |
| Almeida et al. | 2023 | 1.31 | 1.78 | â | 144 | 0.154 | 654* | 0.57 | â |
| Tarricq et al. | 2022 | 1.26 | â | â | 234 | â | â | â | â |
| Dias et al. | 2021 | 1.27 | 1.66 | â | 154 | 0.255 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.31 | 1.02 | â | 219 | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 355 | 0.250 | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit. Silver sample.