FSR 0422

(MWSC 3711)

0.25 UTI

0.0

C_N

0.1

C_dens

0.12

C_C3

0.5

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 17

Radius (P>50% members) 6.5 [arcmin]

C_N 0.0 Sparse
C_dens 0.1 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 0422 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a low-mass, intermediate-age cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~3.06 kpc) differs significantly from the median photometric distance (~1.20 kpc).

Relatively close Moderate extinction Low mass Intermediate age

Data

🔍 Search references for FSR 0422 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	–	348.762	60.859	0.327	-2.948	-1.795	–
Just et al.	2023	348.796	60.806	–	–	–	–
Bica et al.	2019	348.782	60.85	–	–	–	–
Kharchenko et al.	2016	348.796	60.806	–	–	–	–
Dias et al.	2014	348.779	60.85	–	0.18	0.55	–
Kharchenko et al.	2013	348.804	60.81	–	-0.89	-1.93	–
Kharchenko et al.	2012	348.804	60.81	–	-0.89	-1.93	–
Froebrich et al.	2007	348.779	60.85	–	–	–	–
Dias et al.	2002	348.779	60.85	–	-0.89	-1.93	–

💡 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	–	–	–	461	–	11	–	–
Kharchenko et al.	2016	1.20	2.17	–	461	–	–	–	–
Kharchenko et al.	2013	1.20	2.17	–	461	–	–	–	–
Kharchenko et al.	2012	1.20	2.17	–	461	–	–	–	–
Dias et al.	2002	1.20	2.17	–	461	–	–	–	–

Visualization

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