UFMG 16

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C3
N_50
r_50
BA 19 4.7
Summary

UFMG 16 is a sparse, very dense object of high C3 quality. It is located at a relatively close distance from the Sun, above the mid-plane. It is rarely studied in the literature.

This object shares a large percentage of members with a later reported entry.

Warning: contains less than 25 stars with P>0.5 estimated.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Ferreira et al. (2020) 245.05 -44.861 0.734 0.48 -2.347
Dias et al. (2021) 245.084 -44.862 0.737 0.494 -2.352
Almeida et al. (2025) 245.084 -44.862
           
UCC 245.07 -44.868 0.755 0.479 -2.274 -37.705
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

UFMG 16 UCC

Explore data in Colab

Fundamental parameters

Reference Values
Ferreira et al. (2020) E(B-V)=0.5, Dist=1148, logt=8.6
Dias et al. (2021) Av=1.634, Dist=1249, logage=7.918, [Fe/H]=0.138
Almeida et al. (2025) AV=1.634, Dist=1249, logAge=7.918, MassRk=68.3

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 1907 80.0 245.07 -44.89 0.76 0.46 -2.26 -37.71 0.09