FSR 1714

(MWSC 2322)

0.21 UTI

0.0

C_N

0.01

C_dens

0.25

C_C3

0.4

C_lit

1.0

C_dup

N₅₀ (P>50% members) 17

Stellar density (N₅₀/rad) 0.1 [N/pc²]

C3 classification CC

C_N 0.0 Sparse
C_dens 0.01 Very loose
C_C3 0.25 Low quality
C_lit 0.4 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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FSR 1714 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large^* distance, above the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~9.46 kpc) differs significantly from the median photometric distance (~1.61 kpc).

Relatively close Moderate extinction Intermediate age

Data

🔍 Search references for FSR 1714 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–	237.311	-50.604	0.106	-6.263	-4.475	-97.754
Just et al.	2023	237.349	-50.602	–	–	–	–
Bica et al.	2019	237.384	-50.611	–	–	–	–
Kharchenko et al.	2016	237.349	-50.602	–	–	–	–
Dias et al.	2014	237.375	-50.613	–	-4.4	-5.12	–
Kharchenko et al.	2013	237.36	-50.603	–	-4.11	-2.79	–
Froebrich et al.	2007	237.375	-50.613	–	–	–	–
Dias et al.	2002	237.375	-50.613	–	-4.4	-5.12	–

💡 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–	1.61	2.58	–	316	–	127	–	–
Just et al.	2023	–	–	–	316	–	127	–	–
Kharchenko et al.	2016	1.61	2.58	–	316	–	–	–	–
Kharchenko et al.	2013	1.61	2.58	–	316	–	–	–	–
Dias et al.	2002	1.61	2.58	–	316	–	–	–	–

Visualization

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