FSR 0131

(MWSC 3135)

0.23 UTI

0.0

C_N

0.02

C_dens

0.38

C_C3

0.38

C_lit

1.0

C_dup

C3 classification BC

Number of members (P>50%) 10

Radius (P>50% members) 5.9 [arcmin]

C_N 0.0 Sparse
C_dens 0.02 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 0131 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large^* distance, below the mid-plane, affected by very high extinction. It is catalogued as a low-mass, very young cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~5.47 kpc) differs significantly from the median photometric distance (~1.30 kpc).

Relatively close Very high extinction Low mass Very young

Data

🔍 Search references for FSR 0131 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	–	292.686	15.446	0.183	-3.62	-6.519	-5.795
Just et al.	2023	292.672	15.427	–	–	–	–
Bica et al.	2019	292.676	15.429	–	–	–	–
Kharchenko et al.	2016	292.672	15.427	–	–	–	–
Kharchenko et al.	2013	292.678	15.429	–	2.43	-5.43	–
Froebrich et al.	2007	292.675	15.433	–	–	–	–
Dias et al.	2002	292.675	15.433	–	-2.08	-2.85	–

💡 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	–	–	–	5	–	21	–	–
Kharchenko et al.	2016	1.30	8.91	–	5	–	–	–	–
Kharchenko et al.	2013	1.30	8.91	–	5	–	–	–	–
Dias et al.	2002	1.30	8.91	–	5	–	–	–	–

Visualization

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