FoF 1775

(LP 1775)

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.04 0.12 0.0 1.0
C3
N_50
r_50
DC 12 8.3
Summary

FoF 1775 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is rarely studied in the literature.

This object shares a moderate percentage of members with a later 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=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) 316.728 47.089 0.302 -3.354 -4.296 -37.612
Almeida et al. (2025) 316.728 47.089 – – – –
           
UCC 316.738 47.151 0.303 -3.384 -4.346 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

FoF 1775 UCC

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Fundamental parameters

Reference Values
Dias et al. (2021) Av=1.165, Dist=2804, logage=7.478, [Fe/H]=0.144
Almeida et al. (2025) AV=1.165, Dist=2804, logAge=7.478, MassRk=1172.6

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3619 28.0 316.81 47.26 0.31 -3.42 -4.41 – 0.23