CWNU 443

0.04 UTI

0.0

C_N

0.78

C_dens

0.75

C_C3

0.0

C_lit

0.12

C_dup

N₅₀ (P>50% members) 20

Stellar density (N₅₀/rad) 3.9 [N/pc²]

C3 classification BA

C_N 0.0 Sparse
C_dens 0.78 Dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.12 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 443 is a sparse, dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

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

Relatively close Moderate extinction Metal-rich Intermediate age

Data

🔍 Search references for CWNU 443 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–	230.941	-61.971	0.513	-2.554	-2.855	-55.873
He et al.	2022	230.97	-61.979	0.52	-2.56	-2.84	–

💡 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–	2.75	1.68	–	316	0.968	–	–	–
He et al.	2022	2.75	1.68	–	316	0.968	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1628	88.0	230.94	-61.97	0.52	-2.56	-2.85	-55.87	0.39

💡 Note: The % column shows the percentage of members that CWNU 443 shares with each listed object.

Visualization

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