FSR 1345

(MWSC 1531)

0.18 UTI

0.0

C_N

0.04

C_dens

0.25

C_C3

0.31

C_lit

1.0

C_dup

C3 classification CC

Number of members (P>50%) 18

Radius (P>50% members) 9.6 [arcmin]

C_N 0.0 Sparse
C_dens 0.04 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 1345 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate^* distance, well above the mid-plane, affected by very high extinction. It is catalogued as a very young cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~3.36 kpc) differs significantly from the median photometric distance (~2.33 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 Very high extinction Very young

Data

🔍 Search references for FSR 1345 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	–	130.242	-25.381	0.297	-4.634	4.002	66.081
Just et al.	2023	130.204	-25.372	–	–	–	–
Bica et al.	2019	130.243	-25.403	–	–	–	–
Kharchenko et al.	2016	130.204	-25.372	–	–	–	–
Kharchenko et al.	2013	130.21	-25.375	–	-0.15	3.98	–
Froebrich et al.	2007	130.238	-25.402	–	–	–	–

💡 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	–	–	–	9	–	205	–	–
Kharchenko et al.	2016	2.33	5.42	–	9	–	–	–	–
Kharchenko et al.	2013	2.33	5.42	–	9	–	–	–	–

Visualization

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