FoF 1768

(LP 1768)

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C3
N_50
r_50
DC 17 6.9
Summary

FoF 1768 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It is rarely studied in the literature.

This is very likely a unique object, which shares a very small percentage of members with at least one previously reported entry.

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

Warning: the low UTI value and no obvious signs of duplication (C_dup=0.92) 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) 310.634 45.522 0.322 -3.271 -4.763 -29.662
Almeida et al. (2025) 310.634 45.522
           
UCC 310.692 45.504 0.307 -3.265 -4.777 -38.668
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

FoF 1768 UCC

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Fundamental parameters

Reference Values
Dias et al. (2021) Av=2.404, Dist=2525, logage=7.165, [Fe/H]=-0.053
Almeida et al. (2025) AV=2.404, Dist=2525, logAge=7.165, MassRk=1341.2

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 665 8.0 310.6 45.49 0.31 -3.35 -5.14 0.43
Steine 19 8.0 310.59 45.82 0.28 -3.4 -4.89 -23.42 0.06
CWNU 3421 4.0 310.6 45.49 0.31 -3.35 -5.14 0.02