FSR 0414

(MWSC 3688)

0.18 UTI

0.0

C_N

0.03

C_dens

0.12

C_C3

0.38

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 16

Radius (P>50% members) 6.1 [arcmin]

C_N 0.0 Sparse
C_dens 0.03 Very loose
C_C3 0.12 Very low quality
C_lit 0.38 Poorly studied
C_dup 1.0 Unique

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

Overview

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FSR 0414 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large^* distance, above the mid-plane, affected by moderate extinction. It is catalogued as a low-mass, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~6.12 kpc) differs significantly from the median photometric distance (~0.90 kpc).

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Close Moderate extinction Low mass Intermediate age

Data

🔍 Search references for FSR 0414 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	–	345.335	62.978	0.163	-3.113	-1.699	-60.171
Just et al.	2023	345.428	62.979	–	–	–	–
Kharchenko et al.	2016	345.428	62.979	–	–	–	–
Kharchenko et al.	2013	345.435	62.983	–	-1.18	0.27	-23.0
Kharchenko et al.	2012	345.435	62.983	–	-1.31	-0.36	-23.0
Froebrich et al.	2007	345.438	63.021	–	–	–	–
Dias et al.	2002	345.438	63.021	–	0.11	-3.8	-23.0

💡 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	–	–	–	531	–	5	–	–
Kharchenko et al.	2016	0.96	2.06	–	531	–	–	–	–
Kharchenko et al.	2013	0.96	2.06	–	531	–	–	–	–
Kharchenko et al.	2012	0.83	1.94	–	617	–	–	–	–
Dias et al.	2002	0.83	1.94	–	617	–	–	–	–

Visualization

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