FoF 1490

(LP 1490)

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C3
N_50
r_50
DC 79 10.3
Summary

FoF 1490 is a moderately populated, 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.

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) 157.71 -58.263 0.319 -6.807 3.401 0.334
Almeida et al. (2025) 157.71 -58.263
           
UCC 157.755 -58.238 0.334 -6.817 3.4 4.109
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

FoF 1490 UCC

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Fundamental parameters

Reference Values
Dias et al. (2021) Av=1.05, Dist=2449, logage=7.241, [Fe/H]=0.061
Almeida et al. (2025) AV=1.05, Dist=2449, logAge=7.241, MassRk=268.6

Search coordinates in Bayestar19

Cluster region map