FSR 1192

(MWSC 1092)

0.06 UTI

0.0

C_N

0.03

C_dens

0.12

C_C3

0.06

C_lit

1.0

C_dup

N_m (P>50%) 20

Core radius and density 1.6 [pc], 0.1 [pc^-2]

C3 classification DC

C_N 0.0 Sparse
C_dens 0.03 Very loose
C_C3 0.12 Very low quality
C_lit 0.06 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 1192 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large^* distance, below the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~5.95 kpc) differs significantly from the median photometric distance (~2.82 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 Intermediate age

Data

🔍 Search references for FSR 1192 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–	106.439	-11.642	0.168	-0.961	1.07	96.405
Just et al.	2023	106.451	-11.623	–	–	–	–
Kharchenko et al.	2016	106.451	-11.623	–	–	–	–
Kharchenko et al.	2013	106.458	-11.625	–	-1.05	2.42	–
Froebrich et al.	2007	106.458	-11.625	–	–	–	–

💡 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–	2.82	2.43	–	355	–	793	–	–
Just et al.	2023	–	–	–	355	–	793	–	–
Kharchenko et al.	2016	2.82	2.43	–	355	–	–	–	–
Kharchenko et al.	2013	2.82	2.43	–	355	–	–	–	–

Visualization

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