FoF 2000

(LP 2000)

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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

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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

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

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 319.089 57.462 0.714 -3.093 -4.475 -21.357
Almeida et al. 2025 319.079 57.455 – – – –
Almeida et al. 2023 319.049 57.478 – – – –
Tarricq et al. 2022 319.126 57.474 0.704 -3.11 -4.487 –
Dias et al. 2021 319.079 57.455 0.714 -3.113 -4.449 –
Cantat-Gaudin et al. 2020 319.099 57.463 0.71 -3.102 -4.407 –
Liu & Pang 2019 319.038 57.459 0.701 -3.1 -4.402 –

💡 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 – 154 – 413 – –
Almeida et al. 2023 1.31 1.78 – 144 0.154 654* 0.57 –
Tarricq et al. 2022 1.26 – – 234 – – – –
Dias et al. 2021 1.27 1.66 – 154 0.255 – – –
Cantat-Gaudin et al. 2020 1.31 1.02 – 219 – – – –
Liu & Pang 2019 – – – 355 0.250 – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 161 71.9 319.1 57.46 0.71 -3.09 -4.49 -19.99 0.0

💡 Note: The % column shows the percentage of members that FoF 2000 shares with each listed object.

Visualization

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