UPK 12

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C3
N_50
r_50
AA 96 15.5
Summary

UPK 12 is a moderately populated, very dense object of very high C3 quality. It is located at a close distance from the Sun, below the mid-plane. It is well-studied in the literature.

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

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Sim et al. (2019) 288.821 -22.141 0.58 -6.61
Cantat-Gaudin et al. (2020) 288.805 -22.143 1.541 0.579 -6.68
Dias et al. (2021) 288.827 -22.186 1.54 0.617 -6.672 -40.746
Tarricq et al. (2022) 288.907 -22.153 1.498 0.618 -6.631
He et al. (2022) 288.791 -22.165 1.527 0.605 -6.679
Hunt & Reffert (2023) 288.873 -22.078 1.5 0.604 -6.694 -0.255
Cavallo et al. (2024) 288.885 -21.801 1.502
Hunt & Reffert (2024) 288.873 -22.078 1.5 0.604 -6.694 -0.255
Alfonso et al. (2024) 288.816 -21.986 1.463 0.615 -6.715
Almeida et al. (2025) 288.827 -22.186
           
UCC 288.866 -22.142 1.514 0.613 -6.691 4.335
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
Sim et al. (2019) d_pc=644, log(age)=7.9
Cantat-Gaudin et al. (2020) AVNN=0.22, DistPc=628.0, AgeNN=8.3
Dias et al. (2021) Av=0.447, Dist=644, logage=8.121, [Fe/H]=0.017
Tarricq et al. (2022) Dist=616, logAgeNN=8.34
He et al. (2022) A0=0.5, logAge=8.15
Hunt & Reffert (2023) AV50=0.247, diffAV50=0.839, MOD50=8.984, logAge50=8.279
Cavallo et al. (2024) AV50=0.36, dMod50=9.1, logAge50=8.34, [Fe/H]50=0.41
Hunt & Reffert (2024) MassJ=94.7367, MassTot=194.210
Alfonso et al. (2024) AV=0.21994, MOD=8.98996, logAge=8.49581, Z=0.01702
Almeida et al. (2025) AV=0.447, Dist=644, logAge=8.121, MassRk=128.0

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 98 67.7 288.85 -22.13 1.52 0.61 -6.68 4.97 0.0