CWNU 467

0.09 UTI

0.32

C_N

0.61

C_dens

0.5

C_C3

0.0

C_lit

0.31

C_dup

C3 classification BB

Number of members (P>50%) 32

Radius (P>50% members) 5.7 [arcmin]

C_N 0.32 Poorly populated
C_dens 0.61 Moderately dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.31 Possibly duplicate

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

Overview

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CWNU 467 is a poorly populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a relatively close^* distance, above the mid-plane, affected by high extinction. It is catalogued as a metal-rich, very young cluster (see Parameters). It is rarely studied in the literature.

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

(*): The parallax distance estimate (~1.95 kpc) differs significantly from the median photometric distance (~3.24 kpc).

Distant High extinction Metal-rich Very young

Data

🔍 Search references for CWNU 467 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	–	196.355	-61.742	0.512	-4.989	-1.639	–
He et al.	2022	196.529	-61.784	0.52	-4.99	-1.64	–

💡 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
He et al.	2022	3.24	4.02	–	5	0.680	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0589	68.8	196.28	-61.72	0.52	-4.95	-1.59	–	0.36

💡 Note: The % column shows the percentage of members that CWNU 467 shares with each listed object.

Visualization

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