Gulliver 35

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C3
N_50
r_50
AA 77 4.3
Summary

Gulliver 35 is a moderately populated, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It is moderately studied in the literature.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Cantat-Gaudin et al. (2018) 150.379 -58.198 0.405 -6.973 3.967
Soubiran et al. (2018) 150.379 -58.198 86.46
Cantat-Gaudin et al. (2020) 150.379 -58.198 0.405 -6.973 3.967
Dias et al. (2021) 150.35 -58.191 0.411 -6.961 3.982
Hunt & Reffert (2023) 150.379 -58.206 0.43 -6.952 4.004 -12.163
Cavallo et al. (2024) 150.338 -58.181 0.43
Hunt & Reffert (2024) 150.379 -58.206 0.43 -6.952 4.004 -12.163
Almeida et al. (2025) 150.35 -58.191
           
UCC 150.359 -58.198 0.429 -6.941 4.006 -12.245
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=2301.9
Soubiran et al. (2018) dmode=2301.9
Cantat-Gaudin et al. (2020) AVNN=1.05, DistPc=2365.0, AgeNN=8.19
Dias et al. (2021) Av=1.318, Dist=2127, logage=7.839, [Fe/H]=0.267
Hunt & Reffert (2023) AV50=1.329, diffAV50=1.55, MOD50=11.632, logAge50=8.027
Cavallo et al. (2024) AV50=0.91, dMod50=11.57, logAge50=8.65, [Fe/H]50=0.58
Hunt & Reffert (2024) MassJ=479.129, MassTot=493.089
Almeida et al. (2025) AV=1.318, Dist=2127, logAge=7.839, MassRk=146.5

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Cluster region map