Theia 2450

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C3
N_50
r_50
AA 73 10.3
Summary

Theia 2450 is a moderately populated, very dense object of very high 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 likely a duplicate object, which shares a large 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) 202.849 -57.199 0.868 -5.649 -1.375 -23.524
Cavallo et al. (2024) 202.784 -57.202 0.875
Hunt & Reffert (2024) 202.849 -57.199 0.868 -5.649 -1.375 -23.524
           
UCC 202.756 -57.163 0.872 -5.66 -1.375 -24.904
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=0.822, diffAV50=1.241, MOD50=10.175, logAge50=7.617
Cavallo et al. (2024) AV50=1.22, dMod50=10.31, logAge50=7.42, [Fe/H]50=0.13
Hunt & Reffert (2024) MassJ=219.751, MassTot=226.883

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 315 87.7 202.71 -57.17 0.88 -5.67 -1.37 -22.48 0.47
CWWDL 14467 79.5 202.71 -57.17 0.88 -5.66 -1.37 -29.46 0.0