Gulliver 50

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C3
N_50
r_50
AB 76 4.3
Summary

Gulliver 50 is a moderately populated, very dense object of high C3 quality. It is located at a relatively close distance from the Sun, near 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) 181.362 -62.678 0.514 -7.204 1.663
Cantat-Gaudin et al. (2020) 181.362 -62.678 0.514 -7.204 1.663
Dias et al. (2021) 181.382 -62.667 0.523 -7.201 1.667
Hunt & Reffert (2023) 181.361 -62.686 0.546 -7.204 1.668 -27.516
Cavallo et al. (2024) 181.392 -62.676 0.547
Hunt & Reffert (2024) 181.361 -62.686 0.546 -7.204 1.668 -27.516
Almeida et al. (2025) 181.382 -62.667
           
UCC 181.366 -62.683 0.546 -7.205 1.676 -27.374
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=1841.7
Cantat-Gaudin et al. (2020) AVNN=0.94, DistPc=1731.0, AgeNN=7.61
Dias et al. (2021) Av=1.08, Dist=1721, logage=7.738, [Fe/H]=0.207
Hunt & Reffert (2023) AV50=0.726, diffAV50=0.961, MOD50=11.187, logAge50=8.323
Cavallo et al. (2024) AV50=0.85, dMod50=11.16, logAge50=8.63, [Fe/H]50=0.02
Hunt & Reffert (2024) MassJ=394.852, MassTot=405.122
Almeida et al. (2025) AV=1.08, Dist=1721, logAge=7.738, MassRk=321.4

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Cluster region map