Theia 4367

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C3
N_50
r_50
AA 21 1.2
Summary

Theia 4367 is a sparse, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, near 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.

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

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Hunt & Reffert (2023) 176.631 -62.045 0.224 -6.668 1.106 -15.611
Cavallo et al. (2024) 176.628 -62.056 0.227
Hunt & Reffert (2024) 176.631 -62.045 0.224 -6.668 1.106 -15.611
           
UCC 176.636 -62.061 0.216 -6.678 1.094 -0.844
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
Hunt & Reffert (2023) AV50=1.89, diffAV50=1.805, MOD50=12.976, logAge50=8.306
Cavallo et al. (2024) AV50=2.1, dMod50=12.16, logAge50=8.65, [Fe/H]50=-0.56
Hunt & Reffert (2024) MassJ=550.656, MassTot=605.479

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1608 88.0 176.63 -62.06 0.22 -6.68 1.09 -10.18 0.35