Theia 3317

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C3
N_50
r_50
BB 24 4.7
Summary

Theia 3317 is a sparse, moderately dense object of intermediate C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It was recently reported in the literature.

Warning: This is very 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) 138.716 -45.306 0.441 -5.552 4.091
Cavallo et al. (2024) 138.762 -45.317 0.441
Hunt & Reffert (2024) 138.716 -45.306 0.441 -5.552 4.091
           
UCC 138.719 -45.303 0.442 -5.558 4.063
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=1.044, diffAV50=0.549, MOD50=11.674, logAge50=7.894
Cavallo et al. (2024) AV50=1.27, dMod50=11.49, logAge50=7.57, [Fe/H]50=0.05
Hunt & Reffert (2024) MassJ=116.756, MassTot=85.1716

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1854 96.0 138.72 -45.3 0.45 -5.56 4.06 0.32