FSR 0427

(MWSC 3731)

0.24 UTI

0.0

C_N

0.1

C_dens

0.38

C_C3

0.38

C_lit

1.0

C_dup

C3 classification BC

Number of members (P>50%) 19

Radius (P>50% members) 7.7 [arcmin]

C_N 0.0 Sparse
C_dens 0.1 Very loose
C_C3 0.38 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 0427 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate^* distance, below 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 (~2.79 kpc) differs significantly from the median photometric distance (~1.63 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.

Relatively close Moderate extinction Low mass Intermediate age

Data

🔍 Search references for FSR 0427 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	–	352.45	56.913	0.358	-3.844	-1.772	–
Just et al.	2023	352.353	56.941	–	–	–	–
Bica et al.	2019	352.418	56.943	–	–	–	–
Kharchenko et al.	2016	352.353	56.941	–	–	–	–
Kharchenko et al.	2013	352.36	56.945	–	-1.42	-0.11	–
Kharchenko et al.	2012	352.36	56.945	–	-1.42	-0.11	–
Froebrich et al.	2007	352.421	56.948	–	–	–	–

💡 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	–	–	–	398	–	45	–	–
Kharchenko et al.	2016	1.63	2.26	–	398	–	–	–	–
Kharchenko et al.	2013	1.63	2.26	–	398	–	–	–	–
Kharchenko et al.	2012	1.63	2.26	–	398	–	–	–	–

Visualization

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