Gulliver 20

(OCSN 196)

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C3
N_50
r_50
AA 86 37.8
Summary

Gulliver 20 is a moderately populated, dense object of very high C3 quality. It is located at a very close distance from the Sun, above the mid-plane. It is very well-studied in the literature.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Cantat-Gaudin et al. (2018) 273.736 11.082 2.347 1.039 -6.525
Soubiran et al. (2018) 273.736 11.082 -13.92
Bossini et al. (2019) 273.736 11.082
Cantat-Gaudin et al. (2020) 273.736 11.082 2.347 1.039 -6.525
Dias et al. (2021) 273.699 11.105 2.365 1.02 -6.515 -14.879
Tarricq et al. (2022) 273.865 10.416 2.346 1.023 -6.509
He et al. (2022) 273.645 11.039 2.361 1.013 -6.465
Qin et al. (2023) 273.84 11.44 2.38 1.03 -6.55 -13.57
Hunt & Reffert (2023) 273.84 11.438 2.364 1.018 -6.564 -14.434
Cavallo et al. (2024) 273.727 10.969 2.353
Hunt & Reffert (2024) 273.84 11.438 2.364 1.018 -6.564 -14.434
Alfonso et al. (2024) 273.754 10.844 2.311 1.04 -6.507
Almeida et al. (2025) 273.699 11.105
           
UCC 273.754 10.988 2.359 1.023 -6.549 -13.909
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=420.9
Soubiran et al. (2018) dmode=420.9
Bossini et al. (2019) AV=0.149, Dist=7.983, logA=8.289, Fe/H=0.0
Cantat-Gaudin et al. (2020) AVNN=0.25, DistPc=429.0, AgeNN=8.25
Dias et al. (2021) Av=0.338, Dist=422, logage=8.974, [Fe/H]=-0.061
Tarricq et al. (2022) Dist=424, logAgeNN=8.26
He et al. (2022) A0=0.45, logAge=7.9
Qin et al. (2023) E(B-V)=0.16, m-M=8.53, logt=7.95
Hunt & Reffert (2023) AV50=0.192, diffAV50=0.49, MOD50=8.051, logAge50=8.407
Cavallo et al. (2024) AV50=0.53, dMod50=8.16, logAge50=8.09, [Fe/H]50=0.08
Hunt & Reffert (2024) MassJ=73.8268, MassTot=146.912
Alfonso et al. (2024) AV=0.25005, MOD=8.16970, logAge=8.01227, Z=-0.0607
Almeida et al. (2025) AV=0.338, Dist=422, logAge=8.974, MassRk=82.2

Search coordinates in Bayestar19

Cluster region map