Theia 3475

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C3
N_50
r_50
CB 33 8.9
Summary

Theia 3475 is a poorly populated, loose object of low C3 quality. It is located at a relatively close distance from the Sun, above the mid-plane. It was recently reported in the literature.

Warning: This is possibly a duplicated object, which shares a significant percentage of members with at least one previously reported entry.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Hunt & Reffert (2023) 93.198 24.112 0.516 0.146 -1.996 664.493
Cavallo et al. (2024) 93.21 23.9 0.516
Hunt & Reffert (2024) 93.198 24.112 0.516 0.146 -1.996 664.493
           
UCC 93.252 24.106 0.521 0.145 -1.969 664.495
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
Hunt & Reffert (2023) AV50=1.489, diffAV50=2.379, MOD50=11.324, logAge50=8.162
Cavallo et al. (2024) AV50=1.56, dMod50=11.35, logAge50=8.26, [Fe/H]50=-0.34
Hunt & Reffert (2024) MassJ=242.215, MassTot=379.618

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0307 60.6 93.27 24.0 0.52 0.15 -1.93 0.23