FSR 0192

(MWSC 3258)

0.15 UTI

0.0

C_N

0.06

C_dens

0.25

C_C3

0.23

C_lit

1.0

C_dup

N_m (P>50%) 19

Core radius and density 3.0 [pc], 0.3 [pc^-2]

C3 classification CC

C_N 0.0 Sparse
C_dens 0.06 Very loose
C_C3 0.25 Low quality
C_lit 0.23 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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FSR 0192 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature.

⚠️ 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 Very young

Data

🔍 Search references for FSR 0192 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	99999–	301.717	33.811	0.268	-2.296	-4.586	–
Just et al.	2023	301.735	33.821	–	–	–	–
Bica et al.	2019	301.721	33.827	–	–	–	–
Dias et al.	2018	–	–	–	-2.84	-4.68	–
Sampedro et al.	2017	301.717	33.83	–	-3.19	-6.73	–
Kharchenko et al.	2016	301.735	33.821	–	–	–	–
Dias et al.	2014	301.717	33.83	–	-1.57	-6.86	–
Kharchenko et al.	2013	301.74	33.823	–	-1.86	-2.26	–
Froebrich et al.	2007	301.717	33.83	–	–	–	–
Dias et al.	2002	301.717	33.83	–	-1.57	-6.86	–

💡 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]	B_frac	BSS
UCC	99999–	2.65	2.82	–	16	–	681	–	–
Just et al.	2023	–	–	–	16	–	681	–	–
Kharchenko et al.	2016	2.65	2.82	–	16	–	–	–	–
Kharchenko et al.	2013	2.65	2.82	–	16	–	–	–	–
Dias et al.	2002	2.65	2.82	–	16	–	–	–	–

Visualization

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