FSR 0094

(MWSC 3003)

0.22 UTI

0.0

C_N

0.08

C_dens

0.25

C_C3

0.38

C_lit

1.0

C_dup

C3 classification CC

Number of members (P>50%) 14

Radius (P>50% members) 5.1 [arcmin]

C_N 0.0 Sparse
C_dens 0.08 Very loose
C_C3 0.25 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 0094 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane, affected by very high extinction. It is catalogued as a very young cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~4.06 kpc) differs significantly from the median photometric distance (~2.07 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 Very high extinction Very young

Data

🔍 Search references for FSR 0094 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	–	282.457	-0.973	0.246	-1.77	-3.308	9.734
Just et al.	2023	282.462	-1.023	–	–	–	–
Kharchenko et al.	2016	282.462	-1.023	–	–	–	–
Dias et al.	2014	282.458	-1.049	–	-1.85	-4.45	–
Kharchenko et al.	2013	282.469	-1.022	–	0.99	-6.71	–
Froebrich et al.	2007	282.458	-1.049	–	–	–	–
Dias et al.	2002	282.458	-1.049	–	0.99	-6.71	–

💡 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	–	–	–	1	–	255	–	–
Kharchenko et al.	2016	2.07	8.20	–	1	–	–	–	–
Kharchenko et al.	2013	2.07	8.20	–	1	–	–	–	–
Dias et al.	2002	2.07	8.20	–	1	–	–	–	–

Visualization

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