Theia 1796

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C3
N_50
r_50
AB 137 13.5
Summary

Theia 1796 is a rich, very dense object of 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) 290.713 18.709 0.902 -1.035 -6.112 -8.189
Cavallo et al. (2024) 290.806 18.713 0.907
Hunt & Reffert (2024) 290.713 18.709 0.902 -1.035 -6.112 -8.189
           
UCC 290.736 18.697 0.917 -1.031 -6.15 -1.79
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=2.838, diffAV50=2.129, MOD50=10.12, logAge50=7.78
Cavallo et al. (2024) AV50=2.91, dMod50=10.27, logAge50=7.7, [Fe/H]50=0.25
Hunt & Reffert (2024) MassJ=641.802, MassTot=669.934

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 2339 81.8 290.72 18.68 0.92 -1.02 -6.16 -1.96 0.6