Gulliver 57

N_50

r_50

241

7.1

Summary

Gulliver 57 is a rich, very dense object of high C3 quality. It is located at a relatively close distance from the Sun, above the mid-plane. It is well-studied in the literature.

This object shares a moderate 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)	141.203	-48.075	0.701	-6.737	4.085	–
Soubiran et al. (2018)	141.203	-48.075	–	–	–	19.87
Cantat-Gaudin et al. (2020)	141.203	-48.075	0.701	-6.737	4.085	–
Dias et al. (2021)	141.202	-48.085	0.701	-6.721	4.094	5.416
Tarricq et al. (2022)	141.193	-48.051	0.744	-6.7	4.135	–
Hunt & Reffert (2023)	141.201	-48.064	0.736	-6.685	4.133	23.449
Cavallo et al. (2024)	141.194	-48.082	0.736	–	–	–
Hunt & Reffert (2024)	141.201	-48.064	0.736	-6.685	4.133	23.449
Almeida et al. (2025)	141.202	-48.085	–	–	–	–

UCC	141.196	-48.07	0.711	-6.701	4.119	24.935

Galactocentric position

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

1 2 3

Explore data in Colab

Fundamental parameters

Reference	Values
Cantat-Gaudin et al. (2018)	`dmode=1370.5`
Soubiran et al. (2018)	`dmode=1370.5`
Cantat-Gaudin et al. (2020)	`AVNN=2.21, DistPc=1403.0, AgeNN=8.64`
Dias et al. (2021)	`Av=2.724, Dist=1321, logage=7.845, [Fe/H]=0.202`
Tarricq et al. (2022)	`Dist=1351, logAgeNN=8.68`
Hunt & Reffert (2023)	`AV50=2.75, diffAV50=1.877, MOD50=10.574, logAge50=8.365`
Cavallo et al. (2024)	`AV50=2.51, dMod50=10.84, logAge50=8.59, [Fe/H]50=0.64`
Hunt & Reffert (2024)	`MassJ=679.856, MassTot=679.856`
Almeida et al. (2025)	`AV=2.724, Dist=1321, logAge=7.845, MassRk=385.9`

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 11186	27.8	141.21	-48.07	0.74	-6.71	4.14	22.07	0.0