FSR 1751

(MWSC 2398)

0.21 UTI

0.0

C_N

0.2

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) 4.8 [arcmin]

C_N 0.0 Sparse
C_dens 0.2 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

ℹ️

FSR 1751 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 moderate extinction. It is catalogued as an old cluster (see Parameters). It is poorly studied in the literature.

⚠️ 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.

Distant Moderate extinction Old

Data

🔍 Search references for FSR 1751 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	245.991	-32.015	0.328	-5.709	-4.279	-76.125
Just et al.	2023	245.953	-32.009	–	–	–	–
Bica et al.	2019	245.97	-32.008	–	–	–	–
Kharchenko et al.	2016	245.953	-32.009	–	–	–	–
Kharchenko et al.	2013	245.962	-32.01	–	-4.72	-2.04	–
Froebrich et al.	2007	245.963	-32.005	–	–	–	–

💡 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	–	–	–	2600	–	471	–	–
Kharchenko et al.	2016	3.39	1.42	–	2600	–	–	–	–
Kharchenko et al.	2013	3.39	1.42	–	2600	–	–	–	–

Visualization

ℹ️