NGC 2351

(MWSC 1146)

0.20 UTI

0.0

C_N

0.02

C_dens

0.25

C_C3

0.38

C_lit

1.0

C_dup

C3 classification CC

Number of members (P>50%) 12

Radius (P>50% members) 7.9 [arcmin]

C_N 0.0 Sparse
C_dens 0.02 Very loose
C_C3 0.25 Low quality
C_lit 0.38 Poorly studied
C_dup 1.0 Unique

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

Overview

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NGC 2351 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near 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 NGC 2351 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	–	108.398	-10.451	0.229	-1.232	1.524	105.237
Just et al.	2023	108.376	-10.478	–	–	–	–
Loktin & Popova	2017	108.375	-10.48	–	-0.467	0.825	–
Kharchenko et al.	2016	108.376	-10.478	–	–	–	–
Dias et al.	2014	108.379	-10.487	–	-4.02	-1.54	–
Kharchenko et al.	2013	108.382	-10.48	–	-0.43	2.54	–
Dias et al.	2002	108.379	-10.487	–	-4.02	-1.54	–

💡 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	–	–	–	1000	–	530	–	–
Loktin & Popova	2017	4.12	1.89	–	617	–	–	–	–
Kharchenko et al.	2016	5.84	1.62	–	1000	–	–	–	–
Kharchenko et al.	2013	5.84	1.62	–	1000	–	–	–	–
Dias et al.	2002	1.88	2.85	–	240	–	–	–	–

Visualization

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