UBC 390

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C3
N_50
r_50
AB 38 3.7
Summary

UBC 390 is a poorly populated, loose object of high C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is poorly studied in the literature.

Warning: This is 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) 338.707 58.261 0.197 -3.373 -2.156
Cantat-Gaudin et al. (2020) 338.707 58.276 0.194 -3.402 -2.144
Dias et al. (2021) 338.696 58.27 0.209 -3.355 -2.173
Almeida et al. (2025) 338.696 58.27
           
UCC 338.713 58.289 0.22 -3.375 -2.154 -8.544
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=1.58, DistPc=3888.0, AgeNN=7.92
Dias et al. (2021) Av=2.113, Dist=4165, logage=6.912, [Fe/H]=-0.039
Almeida et al. (2025) AV=2.113, Dist=4165, logAge=6.912, MassRk=753.9

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FSR 0377 78.9 338.73 58.3 0.22 -3.29 -2.17 -63.88 0.58