FSR 0341

(MWSC 3586)

0.25 UTI

0.0

C_N

0.13

C_dens

0.12

C_C3

0.5

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 15

Radius (P>50% members) 4.9 [arcmin]

C_N 0.0 Sparse
C_dens 0.13 Very loose
C_C3 0.12 Very low 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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FSR 0341 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate^* distance, below the mid-plane, affected by moderate extinction. It is catalogued as an old cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~3.34 kpc) differs significantly from the median photometric distance (~6.00 kpc).

Very distant Moderate extinction Old

Data

🔍 Search references for FSR 0341 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	–	331.411	53.32	0.299	-3.091	-2.915	–
Just et al.	2023	331.407	53.33	–	–	–	–
Bica et al.	2019	331.393	53.373	–	–	–	–
Kharchenko et al.	2016	331.407	53.33	–	–	–	–
Dias et al.	2014	331.388	53.368	–	-5.15	-5.55	–
Kharchenko et al.	2013	331.413	53.333	–	-3.36	-3.51	–
Kharchenko et al.	2012	331.413	53.333	–	-3.36	-3.51	–
Froebrich et al.	2007	331.387	53.368	–	–	–	–
Dias et al.	2002	331.387	53.368	–	-5.15	-5.55	–

💡 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
Just et al.	2023	–	–	–	1000	–	986	–	–
Kharchenko et al.	2016	6.00	2.17	–	1000	–	–	–	–
Kharchenko et al.	2013	6.00	2.17	–	1000	–	–	–	–
Kharchenko et al.	2012	6.00	2.17	–	1000	–	–	–	–
Dias et al.	2002	6.00	2.17	–	1000	–	–	–	–

Visualization

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