Gulliver 24

(FoF 2126)

N_50

r_50

129

5.5

Summary

Gulliver 24 is a rich, very dense object of high C3 quality. It is located at a relatively close distance from the Sun, near 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)	1.161	62.835	0.636	-3.241	-1.57	–
Soubiran et al. (2018)	1.161	62.835	–	–	–	-31.86
Liu & Pang (2019)	1.148	62.827	0.639	-3.185	-1.48	–
Cantat-Gaudin et al. (2020)	1.161	62.835	0.636	-3.241	-1.57	–
Dias et al. (2021)	1.169	62.843	0.641	-3.254	-1.562	–
Tarricq et al. (2022)	1.121	62.824	0.662	-3.226	-1.58	–
Hunt & Reffert (2023)	1.14	62.836	0.653	-3.204	-1.568	-36.737
Cavallo et al. (2024)	1.135	62.847	0.655	–	–	–
Hunt & Reffert (2024)	1.14	62.836	0.653	-3.204	-1.568	-36.737
Almeida et al. (2025)	1.169	62.843	–	–	–	–

UCC	1.141	62.836	0.654	-3.218	-1.564	-32.7

Galactocentric position

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

1 2 3

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Fundamental parameters

Reference	Values
Cantat-Gaudin et al. (2018)	`dmode=1504.9`
Soubiran et al. (2018)	`dmode=1504.9`
Liu & Pang (2019)	`Age=0.209, Z=-0.25`
Cantat-Gaudin et al. (2020)	`AVNN=1.05, DistPc=1498.0, AgeNN=8.25`
Dias et al. (2021)	`Av=1.367, Dist=1415, logage=8.395, [Fe/H]=0.103`
Tarricq et al. (2022)	`Dist=1443, logAgeNN=8.28`
Hunt & Reffert (2023)	`AV50=1.476, diffAV50=1.423, MOD50=10.791, logAge50=8.102`
Cavallo et al. (2024)	`AV50=1.39, dMod50=11.03, logAge50=8.5, [Fe/H]50=0.42`
Hunt & Reffert (2024)	`MassJ=508.544, MassTot=508.544`
Almeida et al. (2025)	`AV=1.367, Dist=1415, logAge=8.395, MassRk=239.0`

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 10420	58.9	1.15	62.83	0.66	-3.21	-1.56	-32.67	0.0