Gulliver 19

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C3
N_50
r_50
AB 172 6.4
Summary

Gulliver 19 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 is moderately studied in the literature.

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Positions

Reference RA DEC Plx pmRA pmDE Rv
Cantat-Gaudin et al. (2018) 344.19 61.106 0.634 0.893 -2.258
Cantat-Gaudin et al. (2020) 344.19 61.106 0.634 0.893 -2.258
Dias et al. (2021) 344.213 61.11 0.624 0.896 -2.235
Hunt & Reffert (2023) 344.17 61.106 0.646 0.892 -2.307 25.134
Cavallo et al. (2024) 344.188 61.101 0.649
Hunt & Reffert (2024) 344.17 61.106 0.646 0.892 -2.307 25.134
Almeida et al. (2025) 344.213 61.11
           
UCC 344.183 61.104 0.642 0.917 -2.286 8.364
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
Cantat-Gaudin et al. (2018) dmode=1507.9
Cantat-Gaudin et al. (2020) AVNN=3.01, DistPc=1732.0, AgeNN=7.99
Dias et al. (2021) Av=3.404, Dist=1427, logage=7.43, [Fe/H]=0.044
Hunt & Reffert (2023) AV50=3.948, diffAV50=2.935, MOD50=10.851, logAge50=7.596
Cavallo et al. (2024) AV50=3.81, dMod50=11.12, logAge50=7.97, [Fe/H]50=0.6
Hunt & Reffert (2024) MassJ=1024.38, MassTot=1082.20
Almeida et al. (2025) AV=3.404, Dist=1427, logAge=7.43, MassRk=1010.9

Search coordinates in Bayestar19

Cluster region map