FSR 1718

(MWSC 2432)

0.19 UTI

0.0

C_N

0.07

C_dens

0.25

C_C3

0.31

C_lit

1.0

C_dup

C3 classification CC

Number of members (P>50%) 13

Radius (P>50% members) 5.0 [arcmin]

C_N 0.0 Sparse
C_dens 0.07 Very loose
C_C3 0.25 Low quality
C_lit 0.31 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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FSR 1718 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate^* distance, below the mid-plane, affected by low extinction. It is catalogued as a low-mass, old cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~4.05 kpc) differs significantly from the median photometric distance (~2.47 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 Low mass Old

Data

🔍 Search references for FSR 1718 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	–	249.53	-57.101	0.247	-4.505	-7.256	-90.235
Just et al.	2023	249.505	-57.094	–	–	–	–
Bica et al.	2019	249.519	-57.088	–	–	–	–
Kharchenko et al.	2016	249.505	-57.094	–	–	–	–
Kharchenko et al.	2013	249.517	-57.095	–	-6.91	-0.53	–
Froebrich et al.	2007	249.517	-57.087	–	–	–	–

💡 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	–	–	–	3162	–	23	–	–
Kharchenko et al.	2016	2.47	0.39	–	3162	–	–	–	–
Kharchenko et al.	2013	2.47	0.39	–	3162	–	–	–	–

Visualization

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