CWNU 2262

0.19 UTI

0.0

C_N

0.09

C_dens

0.38

C_C3

0.25

C_lit

1.0

C_dup

N₅₀ (P>50% members) 23

Stellar density (N₅₀/rad) 0.4 [N/pc²]

C3 classification CB

C_N 0.0 Sparse
C_dens 0.09 Very loose
C_C3 0.38 Low quality
C_lit 0.25 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 2262 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported 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.

Relatively close Moderate extinction Metal-rich Very young

Palma et al. (2025)
Classified as optical pair P302, along with CWNU_1299.

Cavallo et al. (2024)
Silver sample.

Data

🔍 Search references for CWNU 2262 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–	349.397	61.641	0.338	-4.364	-1.713	-17.681
Hunt & Reffert	2024	349.333	61.606	0.337	-4.367	-1.721	-17.639
Cavallo et al.	2024	349.506	61.652	0.338	–	–	–
Hunt & Reffert	2023	349.333	61.606	0.337	-4.367	-1.721	-17.639
He et al.	2023	349.434	61.624	0.35	-4.347	-1.713	–

💡 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–	2.67	2.98	2.53	18	0.920	405	–	–
Hunt & Reffert	2024	–	–	–	–	–	405⁽¹⁾	–	–
Cavallo et al.	2024	2.96	2.85	–	18	0.920	–	–	–
Hunt & Reffert	2023	2.67	2.98	2.53	9	–	–	–	–
He et al.	2023	2.57	3.45	–	398	–	–	–	–

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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