UBC 492

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C3
N_50
r_50
AB 45 5.6
Summary

UBC 492 is a poorly populated, moderately dense object of high C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It is poorly studied in the literature.

Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Castro-Ginard et al. (2020) 148.74 -50.951 0.393 -6.87 5.023
Cantat-Gaudin et al. (2020) 148.736 -50.951 0.39 -6.86 4.997
Dias et al. (2021) 148.733 -50.949 0.395 -6.874 5.035
Almeida et al. (2025) 148.733 -50.949
           
UCC 148.715 -50.928 0.422 -6.847 5.054 11.126
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

Explore data in Colab

Fundamental parameters

Reference Values
Cantat-Gaudin et al. (2020) AVNN=1.26, DistPc=2627.0, AgeNN=7.77
Dias et al. (2021) Av=1.407, Dist=2252, logage=8.048, [Fe/H]=0.288
Almeida et al. (2025) AV=1.407, Dist=2252, logAge=8.048, MassRk=212.3

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Collinder 213 100.0 148.69 -50.92 0.42 -6.85 5.05 11.13 0.61