Juchert 13

(MWSC 1992; DSH J1201.6-6406; FSR 1600)

0.97 UTI

0.86

C_N

1.0

C_dens

1.0

C_C3

1.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 381

Stellar density (N₅₀/rad) 46.4 [N/pc²]

C3 classification AA

C_N 0.86 Rich
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 1.0 Very well-studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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Juchert 13 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, old cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is very well-studied in the literature.

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

Relatively close Moderate extinction Massive Near-solar metallicity Old

Almeida et al. (2025)
Mass determination: worst fit. Isochrone match: intermediate fit.

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for Juchert 13 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–	180.43	-64.099	0.305	-8.162	0.261	-5.957
Li et al.	2025	180.431	-64.099	0.274	-8.127	0.249	–
Hu & Soubiran	2025	180.419	-64.097	–	–	–	–
Almeida et al.	2025	180.425	-64.099	–	–	–	–
Hunt & Reffert	2024	180.434	-64.101	0.316	-8.163	0.266	-6.105
Cavallo et al.	2024	180.419	-64.097	0.315	–	–	–
Hunt & Reffert	2023	180.434	-64.101	0.316	-8.163	0.266	-6.105
Just et al.	2023	180.411	-64.097	–	–	–	–
Dias et al.	2021	180.425	-64.099	0.272	-8.138	0.246	-6.596
Cantat-Gaudin et al.	2020	180.431	-64.099	0.274	-8.127	0.249	–
Sánchez et al.	2020	180.421	-64.1	–	-8.185	0.328	–
Cantat-Gaudin & Anders	2020	180.431	-64.099	0.274	-8.127	0.249	–
Soubiran et al.	2018	180.431	-64.099	–	–	–	-6.6
Bica et al.	2019	180.42	-64.099	–	–	–	–
Cantat-Gaudin et al.	2018	180.431	-64.099	0.274	-8.127	0.249	–
Kharchenko et al.	2016	180.411	-64.097	–	–	–	–
Dias et al.	2014	180.421	-64.1	–	-5.36	-0.08	–
Kharchenko et al.	2013	180.42	-64.1	–	-15.39	-5.77	–
Kronberger et al.	2006	180.423	-64.1	–	–	–	–
Dias et al.	2002	180.421	-64.1	–	-5.36	-0.08	–

💡 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–	2.82	2.26	1.96	1280	-0.087	1654	–	–
Li et al.	2025	2.75	2.52	–	1439	-0.064	–	–	–
Hu & Soubiran	2025	–	–	–	–	-0.160⁽⁵⁾	–	–	–
Almeida et al.	2025	2.62	1.78	–	3828	–	1654	–	–
Hunt & Reffert	2024	–	–	–	–	–	3604⁽¹⁾	–	–
Cavallo et al.	2024	2.44	2.43	–	1995	-0.110	–	–	–
Hunt & Reffert	2023	2.85	2.21	1.96	1084	–	–	–	–
Just et al.	2023	–	–	–	1000	–	472	–	–
Dias et al.	2021	2.62	1.78	–	3828	0.141	–	–	–
Cantat-Gaudin et al.	2020	3.39	1.74	–	2291	–	–	–	–
Cantat-Gaudin & Anders	2020	3.29	–	–	–	–	–	–	–
Soubiran et al.	2018	3.29	–	–	–	–	–	–	–
Cantat-Gaudin et al.	2018	3.29	–	–	–	–	–	–	–
Kharchenko et al.	2016	2.79	2.58	–	1000	–	–	–	–
Kharchenko et al.	2013	2.79	2.58	–	1000	–	–	–	–
Dias et al.	2002	2.94	2.26	–	1122	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0580	40.2	180.44	-64.1	0.31	-8.18	0.26	-6.06	0.0

💡 Note: The % column shows the percentage of members that Juchert 13 shares with each listed object.

Visualization

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