Loden 1194

(MWSC 2200; OCL 915.3)

0.87 UTI

0.6

C_N

1.0

C_dens

0.75

C_C3

1.0

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 71

Radius (P>50% members) 12.6 [arcmin]

C_N 0.6 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 1.0 Very well-studied
C_dup 1.0 Unique

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

Overview

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Loden 1194 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 low extinction. It is catalogued as a near-solar metallicity, intermediate-age 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.

Close Low extinction Near-solar metallicity Intermediate age

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

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for Loden 1194 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	–	212.013	-59.79	1.346	-7.791	-4.618	-30.27
Li et al.	2025	212.006	-59.786	1.329	-7.762	-4.667	–
Almeida et al.	2025	211.978	-59.79	–	–	–	–
Alfonso et al.	2024	212.09	-59.743	1.306	-7.727	-4.618	–
Hunt & Reffert	2024	212.068	-59.759	1.333	-7.72	-4.636	-30.128
Cavallo et al.	2024	212.101	-59.78	1.34	–	–	–
Hunt & Reffert	2023	212.068	-59.759	1.333	-7.72	-4.636	-30.128
Almeida et al.	2023	211.961	-59.71	–	–	–	–
Just et al.	2023	211.443	-59.743	–	–	–	–
He et al.	2022	212.025	-59.748	1.35	-7.779	-4.593	–
Tarricq et al.	2022	212.026	-59.864	1.353	-7.805	-4.618	–
Dias et al.	2021	211.978	-59.79	1.333	-7.714	-4.668	–
Cantat-Gaudin et al.	2020	212.006	-59.786	1.329	-7.762	-4.667	–
Cantat-Gaudin & Anders	2020	212.006	-59.786	1.329	-7.762	-4.667	–
Bossini et al.	2019	212.006	-59.786	–	–	–	–
Soubiran et al.	2018	212.006	-59.786	–	–	–	-24.79
Bica et al.	2019	211.579	-59.752	–	–	–	–
Cantat-Gaudin et al.	2018	212.006	-59.786	1.329	-7.762	-4.667	–
Kharchenko et al.	2016	211.443	-59.743	–	–	–	–
Dias et al.	2014	211.425	-59.7	–	-3.31	-3.88	–
Kharchenko et al.	2013	211.455	-59.745	–	-7.2	-3.0	2.0
Gozha et al.	2012	211.425	-59.7	–	–	–	–
Piskunov et al.	2008	211.412	-59.714	–	–	–	–
Kharchenko et al.	2007	211.42	-59.7	–	0.18	–	2.0
Kharchenko et al.	2005	211.42	-59.72	–	-10.07	-3.29	999.9

💡 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
Li et al.	2025	0.76	0.69	–	198	0.057	–	–	–
Almeida et al.	2025	0.74	0.84	–	135	–	179	–	–
Alfonso et al.	2024	0.69	0.46	–	273	0.037	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	200*	–	–
Cavallo et al.	2024	0.74	0.43	–	302	0.510	–	–	–
Hunt & Reffert	2023	0.71	0.66	0.62	82	–	–	–	–
Almeida et al.	2023	0.72	0.76	–	236	-0.027	140*	0.47	–
Just et al.	2023	–	–	–	507	–	12	–	–
He et al.	2022	–	0.90	–	63	–	–	–	–
Tarricq et al.	2022	0.69	–	–	251	–	–	–	–
Dias et al.	2021	0.74	0.84	–	135	0.037	–	–	–
Cantat-Gaudin et al.	2020	0.69	0.46	–	251	–	–	–	–
Cantat-Gaudin & Anders	2020	0.74	–	–	–	–	–	–	–
Bossini et al.	2019	0.68	0.34	–	327	0.000	–	–	–
Soubiran et al.	2018	0.74	–	–	–	–	–	–	–
Cantat-Gaudin et al.	2018	0.74	–	–	–	–	–	–	–
Kharchenko et al.	2016	0.67	0.13	–	507	–	–	–	–
Kharchenko et al.	2013	0.67	0.13	–	507	–	–	–	–
Gozha et al.	2012	0.50	–	–	339	–	21	–	–
Piskunov et al.	2008	0.50	0.16	–	339	–	–	–	–
Kharchenko et al.	2005	0.50	0.16	–	339	–	–	–	–

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

Visualization

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