Gulliver 22

0.70 UTI

0.68

C_N

1.0

C_dens

0.75

C_C3

0.55

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 85

Radius (P>50% members) 5.4 [arcmin]

C_N 0.68 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.55 Moderately studied
C_dup 1.0 Unique

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

Overview

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Gulliver 22 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is moderately studied in the literature.

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

Close Moderate extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Silver sample.

Data

🔍 Search references for Gulliver 22 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	–	84.85	26.356	1.352	-1.521	-4.68	6.616
Zhang et al.	2024	84.824	26.345	–	–	–	–
Hunt & Reffert	2024	84.824	26.345	1.331	-1.64	-4.74	7.96
Cavallo et al.	2024	83.985	26.021	1.329	–	–	–
Hunt & Reffert	2023	84.824	26.345	1.331	-1.64	-4.74	7.96
He et al.	2022	84.826	26.337	1.352	-1.419	-4.736	–
Cantat-Gaudin et al.	2020	84.848	26.368	1.257	-1.523	-4.605	–
Cantat-Gaudin & Anders	2020	84.848	26.368	1.257	-1.523	-4.605	–
Monteiro & Dias	2019	84.848	26.368	–	–	–	2.0
Cantat-Gaudin et al.	2018	84.848	26.368	1.257	-1.523	-4.605	–

💡 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
Zhang et al.	2024	–	–	–	–	-0.130*	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	193*	–	–
Cavallo et al.	2024	0.82	1.45	–	6	-0.260	–	–	–
Hunt & Reffert	2023	0.72	0.75	1.82	12	–	–	–	–
He et al.	2022	–	1.40	–	6	–	–	–	–
Cantat-Gaudin & Anders	2020	0.78	–	–	–	–	–	–	–
Monteiro & Dias	2019	0.88	1.33	–	6	0.048	–	–	–
Cantat-Gaudin et al.	2018	0.78	–	–	–	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1428	88.2	84.85	26.35	1.36	-1.52	-4.69	3.44	0.01

💡 Note: The % column shows the percentage of members that Gulliver 22 shares with each listed object.

Visualization

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