Gulliver 17

(FoF 496)

0.75 UTI

0.78

C_N

1.0

C_dens

0.75

C_C3

0.6

C_lit

1.0

C_dup

N₅₀ (P>50% members) 173

Stellar density (N₅₀/rad) 54.5 [N/pc²]

C3 classification AB

C_N 0.78 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.6 Moderately studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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Gulliver 17 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, 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.

Relatively close Moderate extinction Near-solar metallicity Young

Palma et al. (2025)
Classified as optical pair P276, along with Biurakan_2.

Cavallo et al. (2024)
Gold sample.

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

Data

🔍 Search references for Gulliver 17 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	99999–	302.658	35.868	0.555	-1.085	-3.103	12.637
Almeida et al.	2025	302.662	35.875	–	–	–	–
Hunt & Reffert	2024	302.654	35.867	0.558	-1.094	-3.116	7.178
Cavallo et al.	2024	302.666	35.873	0.561	–	–	–
Hunt & Reffert	2023	302.654	35.867	0.558	-1.094	-3.116	7.178
Almeida et al.	2023	302.685	35.87	–	–	–	–
Dias et al.	2021	302.662	35.875	0.557	-1.091	-3.028	–
Cantat-Gaudin et al.	2020	302.654	35.871	0.555	-1.078	-3.029	–
Cantat-Gaudin & Anders	2020	302.654	35.871	0.555	-1.078	-3.029	–
Liu & Pang	2019	302.711	35.845	0.51	-1.661	-4.055	–
Monteiro & Dias	2019	302.654	35.871	–	–	–	2.356
Cantat-Gaudin et al.	2018	302.654	35.871	0.555	-1.078	-3.029	–

💡 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]	B_frac	BSS
UCC	99999–	1.71	1.24	1.25	59	0.115	511	0.58	–
Almeida et al.	2025	1.58	1.24	–	55	–	510	–	–
Hunt & Reffert	2024	–	–	–	–	–	514⁽¹⁾	–	–
Cavallo et al.	2024	1.76	1.39	–	63	0.060	–	–	–
Hunt & Reffert	2023	1.71	1.10	1.25	87	–	–	–	–
Almeida et al.	2023	1.66	1.25	–	104	0.137	511⁽¹⁾	0.58	–
Dias et al.	2021	1.58	1.24	–	55	0.115	–	–	–
Cantat-Gaudin et al.	2020	1.63	0.92	–	69	–	–	–	–
Cantat-Gaudin & Anders	2020	1.71	–	–	–	–	–	–	–
Liu & Pang	2019	–	–	–	29	0.250	–	–	–
Monteiro & Dias	2019	1.92	1.26	–	45	0.029	–	–	–
Cantat-Gaudin et al.	2018	1.71	–	–	–	–	–	–	–

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Teutsch 301	94.2	302.66	35.87	0.55	-1.08	-3.12	12.64	0.17

💡 Note: The % column shows the percentage of members that Gulliver 17 shares with each listed object.

Visualization

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