Gulliver 42

0.65 UTI

0.77

C_N

1.0

C_dens

0.5

C_C3

0.5

C_lit

1.0

C_dup

C3 classification BB

Number of members (P>50%) 160

Radius (P>50% members) 2.1 [arcmin]

C_N 0.77 Rich
C_dens 1.0 Very dense
C_C3 0.5 Intermediate quality
C_lit 0.5 Moderately studied
C_dup 1.0 Unique

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

Overview

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Gulliver 42 is a rich, very dense object of intermediate C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is moderately studied in the literature.

Distant High extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Silver sample.

Data

🔍 Search references for Gulliver 42 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	–	303.934	37.847	0.19	-2.716	-5.496	-27.861
Hunt & Reffert	2024	303.926	37.845	0.201	-2.692	-5.517	-21.001
Cavallo et al.	2024	303.936	37.847	0.191	–	–	–
Hunt & Reffert	2023	303.926	37.845	0.201	-2.692	-5.517	-21.001
Cantat-Gaudin et al.	2020	303.935	37.851	0.181	-2.778	-5.452	–
Cantat-Gaudin & Anders	2020	303.935	37.851	0.181	-2.778	-5.452	–
Monteiro & Dias	2019	303.935	37.851	–	–	–	3.063
Soubiran et al.	2018	303.935	37.851	–	–	–	0.41
Cantat-Gaudin et al.	2018	303.935	37.851	0.181	-2.778	-5.452	–

💡 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
Hunt & Reffert	2024	–	–	–	–	–	936*	–	–
Cavallo et al.	2024	4.33	4.19	–	174	-0.190	–	–	–
Hunt & Reffert	2023	4.18	3.18	2.16	135	–	–	–	–
Cantat-Gaudin & Anders	2020	4.76	–	–	–	–	–	–	–
Monteiro & Dias	2019	9.94	3.03	–	6	0.023	–	–	–
Soubiran et al.	2018	4.76	–	–	–	–	–	–	–
Cantat-Gaudin et al.	2018	4.76	–	–	–	–	–	–	–

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

Visualization

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