UFMG 41

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C3
N_50
r_50
AB 51 2.4
Summary

UFMG 41 is a moderately populated, very dense object of high C3 quality. It is located at a relatively close distance from the Sun, near the mid-plane. It is poorly studied in the literature.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Ferreira et al. (2020) 235.14 -55.729 0.503 -1.026 -1.897
Dias et al. (2021) 235.135 -55.75 0.506 -1.017 -1.895
Hunt & Reffert (2023) 235.117 -55.754 0.548 -1.043 -1.845 -28.67
Cavallo et al. (2024) 235.128 -55.758 0.546
Hunt & Reffert (2024) 235.117 -55.754 0.548 -1.043 -1.845 -28.67
Almeida et al. (2025) 235.135 -55.75
           
UCC 235.116 -55.75 0.534 -1.053 -1.884 -28.669
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

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Fundamental parameters

Reference Values
Ferreira et al. (2020) E(B-V)=1.26, Dist=1445, logt=8.2
Dias et al. (2021) Av=3.148, Dist=1767, logage=7.861, [Fe/H]=0.194
Hunt & Reffert (2023) AV50=3.373, diffAV50=1.732, MOD50=11.181, logAge50=7.947
Cavallo et al. (2024) AV50=3.76, dMod50=11.33, logAge50=7.87, [Fe/H]50=-0.02
Hunt & Reffert (2024) MassJ=421.328, MassTot=421.328
Almeida et al. (2025) AV=3.148, Dist=1767, logAge=7.861, MassRk=155.9

Search coordinates in Bayestar19

Cluster region map