Gulliver 41

0.57 UTI

0.66

C_N

1.0

C_dens

0.75

C_C3

0.25

C_lit

0.98

C_dup

C3 classification AB

Number of members (P>50%) 81

Radius (P>50% members) 1.9 [arcmin]

C_N 0.66 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.25 Poorly studied
C_dup 0.98 Unique

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

Overview

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Gulliver 41 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature, with no articles listed in the last 6 years.

Note: This is a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

Very distant High extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for Gulliver 41 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	–	277.716	-12.427	0.181	-1.703	-4.771	58.103
Cantat-Gaudin et al.	2020	277.718	-12.429	0.171	-1.79	-4.709	–
Cantat-Gaudin & Anders	2020	277.718	-12.429	0.171	-1.79	-4.709	–
Monteiro & Dias	2019	277.718	-12.429	–	–	–	3.239
Cantat-Gaudin et al.	2018	277.718	-12.429	0.171	-1.79	-4.709	–

💡 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
Cantat-Gaudin & Anders	2020	5.00	–	–	–	–	–	–	–
Monteiro & Dias	2019	7.33	3.91	–	196	0.049	–	–	–
Cantat-Gaudin et al.	2018	5.00	–	–	–	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Ruprecht 141	2.5	277.82	-12.33	0.33	-1.47	-4.25	20.69	0.35

💡 Note: The % column shows the percentage of members that Gulliver 41 shares with each listed object.

Visualization

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