Gulliver 27

N_50

r_50

121

2.5

Summary

Gulliver 27 is a rich, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is well-studied in the literature.

Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry.

Search object in SciX | Simbad

Positions

Reference	RA	DEC	Plx	pmRA	pmDE	Rv
Cantat-Gaudin et al. (2018)	146.088	-54.117	0.322	-4.658	3.467	–
Soubiran et al. (2018)	146.088	-54.117	–	–	–	18.53
Cantat-Gaudin et al. (2020)	146.088	-54.117	0.322	-4.658	3.467	–
Dias et al. (2021)	146.08	-54.115	0.322	-4.662	3.467	18.368
Rain et al. (2021)	146.088	-54.117	0.322	-4.658	3.467	–
Hunt & Reffert (2023)	146.088	-54.112	0.333	-4.656	3.442	16.662
Cavallo et al. (2024)	146.089	-54.108	0.332	–	–	–
Almeida et al. (2025)	146.08	-54.115	–	–	–	–
Hu & Soubiran (2025)	146.089	-54.108	–	–	–	–

UCC	146.085	-54.109	0.331	-4.645	3.446	17.293

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=2850.4`
Soubiran et al. (2018)	`dmode=2850.4`
Cantat-Gaudin et al. (2020)	`AVNN=1.09, DistPc=2716.0, AgeNN=8.78`
Dias et al. (2021)	`Av=1.67, Dist=2530, logage=8.535, [Fe/H]=0.022`
Rain et al. (2021)	`E(B-V)=0.6, Dist=2850.4, log(Age)=8.5, NBSS=0`
Hunt & Reffert (2023)	`AV50=1.449, diffAV50=0.933, MOD50=12.12, logAge50=8.422`
Cavallo et al. (2024)	`AV50=1.42, dMod50=11.94, logAge50=8.74, [Fe/H]50=0.08`
Almeida et al. (2025)	`AV=1.67, Dist=2530, logAge=8.535, MassRk=387.2`
Hu & Soubiran (2025)	`MA22=-0.11, MA23f=-0.36, MA23g=-0.1, MZ23=-0.19, MK24=-0.2, MF24=-0.3`

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Teutsch 68	81.0	146.08	-54.11	0.33	-4.64	3.44	17.29	0.65