FoF 1725

(LP 1725)

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C3
N_50
r_50
DB 20 5.3
Summary

FoF 1725 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) 299.269 29.963 0.25 -2.663 -5.072 1.728
Almeida et al. (2025) 299.269 29.963
           
UCC 299.264 29.949 0.21 -2.676 -5.078 -38.657
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

FoF 1725 UCC

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Fundamental parameters

Reference Values
Dias et al. (2021) Av=2.259, Dist=3565, logage=8.883, [Fe/H]=0.118
Almeida et al. (2025) AV=2.259, Dist=3565, logAge=8.883, MassRk=2661.5

Search coordinates in Bayestar19

Cluster region map