FSR 0941

(MWSC 846)

0.90 UTI

0.75

C_N

1.0

C_dens

0.75

C_C3

1.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 104

Stellar density (N₅₀/rad) 7.4 [N/pc²]

C3 classification AB

C_N 0.75 Rich
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

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

Overview

ℹ️

FSR 0941 is a rich, very dense object of high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is very well-studied in the literature.

Distant Moderate extinction Massive Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

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

Data

🔍 Search references for FSR 0941 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	95.443	15.77	0.194	0.774	0.12	22.054
Li et al.	2025	95.445	15.776	0.198	0.758	0.139	–
Hu & Soubiran	2025	95.435	15.767	–	–	–	–
Almeida et al.	2025	95.456	15.765	–	–	–	–
Zhang et al.	2024	95.432	15.767	–	–	–	–
Hunt & Reffert	2024	95.432	15.767	0.198	0.782	0.122	21.023
Cavallo et al.	2024	95.435	15.767	0.199	–	–	–
He et al.	2023	95.4	15.72	0.244	-0.033	-0.217	–
Hunt & Reffert	2023	95.432	15.767	0.198	0.782	0.122	21.023
Just et al.	2023	95.438	15.734	–	–	–	–
Dias et al.	2021	95.456	15.765	0.153	0.874	0.135	–
Spina et al.	2021	95.442	15.775	0.181	0.851	0.159	–
Cantat-Gaudin et al.	2020	95.445	15.776	0.198	0.758	0.139	–
Sánchez et al.	2020	95.446	15.74	–	0.788	0.183	–
Zhong et al.	2020	95.445	15.776	–	0.758	0.139	34.981
Cantat-Gaudin & Anders	2020	95.445	15.776	0.198	0.758	0.139	–
Bica et al.	2019	95.46	15.769	–	–	–	–
Cantat-Gaudin et al.	2018	95.445	15.776	0.198	0.758	0.139	–
Kharchenko et al.	2016	95.438	15.734	–	–	–	–
Dias et al.	2014	95.446	15.74	–	0.91	-0.6	–
Kharchenko et al.	2013	95.446	15.733	–	-0.83	-4.93	–
Froebrich et al.	2007	95.463	15.766	–	–	–	–
Dias et al.	2002	95.446	15.74	–	0.91	-0.6	–

💡 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–	4.385	2.55	1.67	468	-0.215	1125	–	–
Li et al.	2025	4.29	2.56	–	613	-0.053	–	–	–
Hu & Soubiran	2025	–	–	–	–	-0.150⁽⁵⁾	–	–	–
Almeida et al.	2025	3.98	2.55	–	601	–	606	–	–
Zhang et al.	2024	–	–	–	–	-0.284⁽¹⁾	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	1457⁽¹⁾	–	–
Cavallo et al.	2024	3.94	2.59	–	631	0.070	–	–	–
He et al.	2023	3.55	2.40	–	200	–	–	–	–
Hunt & Reffert	2023	4.08	2.46	1.67	453	–	–	–	–
Just et al.	2023	–	–	–	462	–	1125	–	–
Dias et al.	2021	3.98	2.55	–	601	-0.221	–	–	–
Spina et al.	2021	4.44	–	–	468	-0.277⁽²⁰⁾	–	–	–
Cantat-Gaudin et al.	2020	4.37	2.23	–	468	–	–	–	–
Zhong et al.	2020	4.61	2.71	–	8665	-0.283	–	–	–
Cantat-Gaudin & Anders	2020	4.40	–	–	–	–	–	–	–
Cantat-Gaudin et al.	2018	4.40	–	–	–	–	–	–	–
Kharchenko et al.	2016	4.61	2.71	–	462	–	–	–	–
Kharchenko et al.	2013	4.61	2.71	–	462	–	–	–	–
Dias et al.	2002	5.80	2.48	–	501	-0.210	–	–	–

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

Visualization

ℹ️

1 2 3