CWNU 3067

0.01 UTI

0.6

C_N

0.15

C_dens

1.0

C_C3

0.0

C_lit

0.03

C_dup

N_m (P>50%) 71

Core radius and density 3.8 [pc], 0.7 [pc^-2]

C3 classification AA

C_N 0.6 Moderately populated
C_dens 0.15 Very loose
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.03 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 3067 is a moderately populated, very loose object of very high 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 was recently reported in the literature.

⚠️ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

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

Distant Moderate extinction Old Contains BSS

Data

🔍 Search references for CWNU 3067 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–	71.693	60.877	0.228	0.553	-0.102	-18.761
Cui et al.	2025	71.68	60.876	0.23	0.56	-0.11	–
He et al.	2023	71.689	60.873	0.23	0.559	-0.11	-18.76

💡 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–	3.16	1.755	–	1682	–	–	–	1
Cui et al.	2025	–	1.76	–	1778	–	–	–	1⁽¹⁾
He et al.	2023	3.16	1.75	–	1585	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 3218	97.2	71.69	60.87	0.24	0.55	-0.1	-18.76	0.09
CWWL 3078	88.7	71.69	60.88	0.23	0.55	-0.1	-18.76	0.39

💡 Note: The % column shows the percentage of members that CWNU 3067 shares with each listed object.

Visualization

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