Theia 1082

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C3
N_50
r_50
CC 23 16.7
Summary

Theia 1082 is a sparse, loose object of low C3 quality. It is located at a close distance from the Sun, above the mid-plane. It was recently reported in the literature.

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

Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Hunt & Reffert (2023) 193.652 -58.96 1.179 -9.883 -3.399 -20.713
Cavallo et al. (2024) 192.84 -58.986 1.179
Hunt & Reffert (2024) 193.652 -58.96 1.179 -9.883 -3.399 -20.713
           
UCC 193.248 -59.062 1.194 -9.867 -3.502 -22.305
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

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Fundamental parameters

Reference Values
Hunt & Reffert (2023) AV50=0.36, diffAV50=0.517, MOD50=9.526, logAge50=8.2
Cavallo et al. (2024) AV50=0.72, dMod50=9.57, logAge50=8.03, [Fe/H]50=0.17
Hunt & Reffert (2024) MassJ=89.9711, MassTot=215.888

Search coordinates in Bayestar19

Cluster region map