FoF 1809

(LP 1809)

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0.42 UTI
0.74
CN
1.0
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 7.3 [N/pc2]
  • CN 0.74 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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FoF 1809 is a moderately populated, very dense object of low 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 (see Parameters). It is rarely studied in the literature.

Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.

Almeida et al. (2025)
Mass determination: good fit. Isochrone match: intermediate 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 99999– 334.709 57.432 0.325 -4.398 -3.551 -60.958
Almeida et al. 2025 334.707 57.426 – – – –
Almeida et al. 2023 334.712 57.426 – – – –
Dias et al. 2021 334.707 57.426 0.342 -4.359 -3.434 -84.263

💡 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 99999– 2.71 2.73 – 441 0.038 686 0.67 –
Almeida et al. 2025 2.71 2.73 – 441 – 886 – –
Almeida et al. 2023 2.60 2.86 – 218 -0.016 487(1) 0.67 –
Dias et al. 2021 2.71 2.73 – 441 0.092 – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 2547 78.8 334.72 57.43 0.32 -4.4 -3.57 -66.8 0.03
OC 0175 45.5 334.72 57.44 0.32 -4.39 -3.59 -72.64 0.0

💡 Note: The % column shows the percentage of members that FoF 1809 shares with each listed object.

Visualization

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