FoF 1798

(LP 1798)

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C3
N_50
r_50
BC 21 5.9
Summary

FoF 1798 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is poorly 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) 331.931 55.618 0.248 -3.345 -2.965 -65.721
He et al. (2023) 331.835 55.646 0.188 -3.253 -2.735 -67.26
Almeida et al. (2025) 331.931 55.618
           
UCC 331.982 55.593 0.247 -3.358 -2.982 -60.738
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

FoF 1798 UCC

Explore data in Colab

Fundamental parameters

Reference Values
Dias et al. (2021) Av=1.893, Dist=3265, logage=7.064, [Fe/H]=-0.153
He et al. (2023) A0=2.6, m-M=13.15, logA=7.6
Almeida et al. (2025) AV=1.893, Dist=3265, logAge=7.064, MassRk=1255.4

Search coordinates in Bayestar19

Cluster region map