Gulliver 39

N_50

r_50

101

3.3

Summary

Gulliver 39 is a rich, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It is well-studied in the literature.

This object shares a significant percentage of members with a later reported entry.

Search object in SciX | Simbad

Positions

Reference	RA	DEC	Plx	pmRA	pmDE	Rv
Cantat-Gaudin et al. (2018)	163.697	-58.05	0.335	-4.407	1.274	–
Soubiran et al. (2018)	163.697	-58.05	–	–	–	-15.98
Cantat-Gaudin et al. (2020)	163.697	-58.05	0.335	-4.407	1.274	–
Dias et al. (2021)	163.696	-58.051	0.334	-4.403	1.275	-15.852
Rain et al. (2021)	163.697	-58.05	0.335	-4.407	1.274	–
Hunt & Reffert (2023)	163.703	-58.048	0.371	-4.462	1.252	-2.766
Cavallo et al. (2024)	163.73	-58.054	0.37	–	–	–
Hunt & Reffert (2024)	163.703	-58.048	0.371	-4.462	1.252	-2.766
Almeida et al. (2025)	163.696	-58.051	–	–	–	–
Hu & Soubiran (2025)	163.73	-58.054	–	–	–	–

UCC	163.71	-58.053	0.36	-4.461	1.253	-13.219

Galactocentric position

How are the galactocentric plots generated?

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Estimated members

1 2 3

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Fundamental parameters

Reference	Values
Cantat-Gaudin et al. (2018)	`dmode=2747.5`
Soubiran et al. (2018)	`dmode=2747.5`
Cantat-Gaudin et al. (2020)	`AVNN=1.38, DistPc=2536.0, AgeNN=8.79`
Dias et al. (2021)	`Av=1.623, Dist=2389, logage=8.89, [Fe/H]=-0.054`
Rain et al. (2021)	`E(B-V)=0.23, Dist=2747.5, log(Age)=8.91, NBSS=0`
Hunt & Reffert (2023)	`AV50=1.574, diffAV50=1.922, MOD50=11.973, logAge50=8.72`
Cavallo et al. (2024)	`AV50=1.49, dMod50=11.91, logAge50=8.92, [Fe/H]50=0.3`
Hunt & Reffert (2024)	`MassJ=840.909, MassTot=841.676`
Almeida et al. (2025)	`AV=1.623, Dist=2389, logAge=8.89, MassRk=89.9`
Hu & Soubiran (2025)	`MA22=-0.17, MA23f=-0.37, MA23g=-0.02, MZ23=-0.41, MK24=-0.29, MF24=-0.28`

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 2197	62.4	163.71	-58.05	0.36	-4.47	1.25	-12.49	0.0