FoF 1989

(LP 1989)

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.06 0.25 0.0 1.0
C3
N_50
r_50
CC 20 7.0
Summary

FoF 1989 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It is rarely studied in the literature.

Warning: contains less than 25 stars with P>0.5 estimated.

Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2021) 125.014 -30.685 0.244 -2.504 2.364 46.668
Almeida et al. (2025) 125.014 -30.685 – – – –
           
UCC 125.05 -30.663 0.247 -2.491 2.349 78.731
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

FoF 1989 UCC

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Fundamental parameters

Reference Values
Dias et al. (2021) Av=0.872, Dist=3654, logage=8.914, [Fe/H]=-0.142
Almeida et al. (2025) AV=0.872, Dist=3654, logAge=8.914, MassRk=1170.2

Search coordinates in Bayestar19

Cluster region map