FoF 1728

(LP 1728)

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C3
N_50
r_50
BB 15 5.6
Summary

FoF 1728 is a sparse, very loose object of intermediate C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It is rarely studied in the literature.

This object shares a moderate percentage of members with 2 later reported entries.

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) 298.765 29.955 0.24 -2.365 -4.895 1.422
Almeida et al. (2025) 298.765 29.955
           
UCC 298.733 29.914 0.231 -2.411 -4.874
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

FoF 1728 UCC

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Fundamental parameters

Reference Values
Dias et al. (2021) Av=2.056, Dist=3806, logage=7.053, [Fe/H]=0.152
Almeida et al. (2025) AV=2.056, Dist=3806, logAge=7.053, MassRk=1780.2

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 529 40.0 298.67 29.79 0.23 -2.46 -4.84 0.26
CWNU 4799 36.0 298.67 29.8 0.23 -2.45 -4.85 0.04