CWNU 3142

0.19 UTI

0.33

C_N

0.26

C_dens

0.38

C_C3

0.0

C_lit

1.0

C_dup

N_m (P>50%) 33

Core radius and density 1.6 [pc], 1.3 [pc^-2]

C3 classification BC

C_N 0.33 Poorly populated
C_dens 0.26 Loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 3142 is a poorly populated, 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 old cluster (see Parameters). It was recently reported in the literature.

Note: This object contains blue stragglers according to at least one source.

⚠️ 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.

Very distant Moderate extinction Old Contains BSS

Data

🔍 Search references for CWNU 3142 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–	1.293	63.339	0.158	-0.708	-0.758	-70.783
Cui et al.	2025	1.307	63.336	0.16	-0.74	-0.78	–
He et al.	2023	1.3	63.338	0.162	-0.736	-0.775	-70.78

💡 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–	6.17	2.36	–	2406	–	–	–	6
Cui et al.	2025	–	2.32	–	2818	–	–	–	6⁽¹⁾
He et al.	2023	6.17	2.40	–	1995	–	–	–	–

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

Visualization

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