FSR 1294

(MWSC 1359)

0.13 UTI

0.0

C_N

0.02

C_dens

0.25

C_C3

0.19

C_lit

1.0

C_dup

N_m (P>50%) 18

Core radius and density 5.2 [pc], 0.1 [pc^-2]

C3 classification CC

C_N 0.0 Sparse
C_dens 0.02 Very loose
C_C3 0.25 Low quality
C_lit 0.19 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 1294 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate^* distance, above the mid-plane, affected by low extinction. It is catalogued as an old cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~3.75 kpc) differs significantly from the median photometric distance (~2.12 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 Low extinction Old

Data

🔍 Search references for FSR 1294 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–	117.764	-22.134	0.267	-2.084	1.679	81.413
Just et al.	2023	117.782	-22.108	–	–	–	–
Bica et al.	2019	117.781	-22.134	–	–	–	–
Sampedro et al.	2017	117.779	-22.131	–	-4.48	-1.3	–
Kharchenko et al.	2016	117.782	-22.108	–	–	–	–
Dias et al.	2014	117.779	-22.131	–	1.41	-1.63	–
Kharchenko et al.	2013	117.787	-22.11	–	-4.24	0.76	–
Froebrich et al.	2007	117.779	-22.131	–	–	–	–
Dias et al.	2002	117.779	-22.131	–	-4.24	0.76	–

💡 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–	2.12	0.66	–	1641	–	137	–	–
Just et al.	2023	–	–	–	1641	–	137	–	–
Kharchenko et al.	2016	2.12	0.66	–	1641	–	–	–	–
Kharchenko et al.	2013	2.12	0.66	–	1641	–	–	–	–
Dias et al.	2002	2.12	0.66	–	1641	–	–	–	–

Visualization

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