UFMG 90

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C3
N_50
r_50
AA 92 4.5
Summary

UFMG 90 is a moderately populated, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is poorly studied in the literature.

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

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Ferreira et al. (2021) 270.655 -25.83 0.44 0.455 -0.083
Hunt & Reffert (2023) 270.64 -25.816 0.471 0.588 0.008 -38.703
Cavallo et al. (2024) 270.644 -25.818 0.474
Hunt & Reffert (2024) 270.64 -25.816 0.471 0.588 0.008 -38.703
           
UCC 270.637 -25.819 0.458 0.558 -0.02 -48.969
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
Ferreira et al. (2021) E(B-V)=1.15, Dmod=10.85, logt=8.9
Hunt & Reffert (2023) AV50=3.87, diffAV50=2.755, MOD50=11.512, logAge50=8.167
Cavallo et al. (2024) AV50=4.3, dMod50=11.02, logAge50=8.42, [Fe/H]50=-1.01
Hunt & Reffert (2024) MassJ=1668.27, MassTot=1795.83

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2859 28.3 270.64 -25.81 0.46 0.59 -0.02 -48.4 0.0