Gulliver 14

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C3
N_50
r_50
AA 65 7.4
Summary

Gulliver 14 is a moderately populated, very dense object of very high C3 quality. It is located at a relatively close distance from the Sun, near the mid-plane. It is well-studied in the literature.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Cantat-Gaudin et al. (2018) 259.928 -36.785 0.745 -3.719 -4.792
Soubiran et al. (2018) 259.928 -36.785 -13.36
Cantat-Gaudin et al. (2020) 259.928 -36.785 0.745 -3.719 -4.792
Dias et al. (2021) 259.915 -36.763 0.741 -3.733 -4.779
Tarricq et al. (2022) 259.956 -36.702 0.748 -3.751 -4.795
Hunt & Reffert (2023) 259.946 -36.708 0.763 -3.759 -4.756 -16.263
Cavallo et al. (2024) 259.928 -36.738 0.76
Hunt & Reffert (2024) 259.946 -36.708 0.763 -3.759 -4.756 -16.263
Almeida et al. (2025) 259.915 -36.763
Hu & Soubiran (2025) 259.928 -36.738
           
UCC 259.925 -36.742 0.763 -3.761 -4.79 -15.558
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=1291.5
Soubiran et al. (2018) dmode=1291.5
Cantat-Gaudin et al. (2020) AVNN=1.63, DistPc=1247.0, AgeNN=8.78
Dias et al. (2021) Av=2.003, Dist=1262, logage=8.535, [Fe/H]=0.17
Tarricq et al. (2022) Dist=1204, logAgeNN=8.82
Hunt & Reffert (2023) AV50=1.934, diffAV50=0.993, MOD50=10.467, logAge50=8.595
Cavallo et al. (2024) AV50=1.81, dMod50=10.28, logAge50=8.92, [Fe/H]50=0.09
Hunt & Reffert (2024) MassJ=315.694, MassTot=327.343
Almeida et al. (2025) AV=2.003, Dist=1262, logAge=8.535, MassRk=172.8
Hu & Soubiran (2025) MA22=-0.08, MA23f=-0.06, MA23g=0.19, MZ23=0.01, MK24=-0.07, MF24=-0.23

Search coordinates in Bayestar19

Cluster region map