CWNU 3232

0.04 UTI

0.29

C_N

0.24

C_dens

0.25

C_C3

0.0

C_lit

0.24

C_dup

C3 classification DB

Number of members (P>50%) 29

Radius (P>50% members) 4.1 [arcmin]

C_N 0.29 Poorly populated
C_dens 0.24 Very loose
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.24 Likely duplicate

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

Overview

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CWNU 3232 is a poorly populated, 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 an intermediate-age cluster (see Parameters). It was recently reported 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.

Distant Moderate extinction Intermediate age

Data

🔍 Search references for CWNU 3232 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	–	115.655	-20.68	0.244	-1.665	2.542	–
He et al.	2023	115.654	-20.683	0.23	-1.684	2.547	88.29

💡 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.	2023	3.47	1.10	–	501	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1886	75.9	115.66	-20.69	0.24	-1.68	2.54	–	0.19

💡 Note: The % column shows the percentage of members that CWNU 3232 shares with each listed object.

Visualization

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