Gulliver 31

0.80 UTI

0.75

C_N

1.0

C_dens

0.75

C_C3

0.75

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 104

Radius (P>50% members) 4.1 [arcmin]

C_N 0.75 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.75 Well-studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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Gulliver 31 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is well-studied in the literature.

Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Intermediate age

Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit. Silver sample.

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for Gulliver 31 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	301.914	38.244	0.387	-1.461	-3.174	-15.243
Li et al.	2025	301.912	38.232	0.396	-1.5	-3.113	–
Almeida et al.	2025	301.911	38.24	–	–	–	–
Zhang et al.	2024	301.885	38.247	–	–	–	–
Hunt & Reffert	2024	301.885	38.247	0.381	-1.474	-3.174	-13.942
Cavallo et al.	2024	301.919	38.259	0.383	–	–	–
Hunt & Reffert	2023	301.885	38.247	0.381	-1.474	-3.174	-13.942
Almeida et al.	2023	301.917	38.252	–	–	–	–
Dias et al.	2021	301.911	38.24	0.395	-1.491	-3.113	–
Cantat-Gaudin et al.	2020	301.912	38.232	0.396	-1.5	-3.113	–
Cantat-Gaudin & Anders	2020	301.912	38.232	0.396	-1.5	-3.113	–
Monteiro & Dias	2019	301.912	38.232	–	–	–	2.212
Soubiran et al.	2018	301.912	38.232	–	–	–	-11.45
Cantat-Gaudin et al.	2018	301.912	38.232	0.396	-1.5	-3.113	–

💡 Note: The UCC values are estimated from its identified members.

Reference	Year	Dist [kpc]	Av [mag]	DAv [mag]	Age [Myr]	[Fe/H] [dex]	Mass [Msun]	Bfr	BSS
Li et al.	2025	2.05	1.34	–	194	0.052	–	–	–
Almeida et al.	2025	2.14	1.65	–	39	–	354	–	–
Zhang et al.	2024	–	–	–	–	-0.112*	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	683*	–	–
Cavallo et al.	2024	2.62	1.37	–	234	0.820	–	–	–
Hunt & Reffert	2023	2.38	1.58	1.51	136	–	–	–	–
Almeida et al.	2023	2.13	1.56	–	177	0.112	371*	0.62	–
Dias et al.	2021	2.14	1.65	–	39	0.148	–	–	–
Cantat-Gaudin et al.	2020	2.49	1.10	–	145	–	–	–	–
Cantat-Gaudin & Anders	2020	2.35	–	–	–	–	–	–	–
Monteiro & Dias	2019	3.00	1.85	–	51	0.049	–	–	–
Soubiran et al.	2018	2.35	–	–	–	–	–	–	–
Cantat-Gaudin et al.	2018	2.35	–	–	–	–	–	–	–

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 12276	51.9	301.91	38.24	0.39	-1.46	-3.18	-18.73	0.0

💡 Note: The % column shows the percentage of members that Gulliver 31 shares with each listed object.

Visualization

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