CWNU 332

0.05 UTI

0.28

C_N

1.0

C_dens

0.25

C_C3

0.0

C_lit

0.18

C_dup

C3 classification DB

Number of members (P>50%) 28

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

C_N 0.28 Poorly populated
C_dens 1.0 Very dense
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.18 Likely duplicate

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

Overview

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CWNU 332 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a metal-rich, young 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 Low extinction Metal-rich Young

Data

🔍 Search references for CWNU 332 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	–	105.831	-12.651	0.777	-0.55	-0.378	-29.103
He et al.	2022	105.83	-12.666	0.78	-0.56	-0.38	–

💡 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	1.23	0.84	–	50	0.680	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0376	82.1	105.83	-12.66	0.77	-0.57	-0.36	-29.1	0.4

💡 Note: The % column shows the percentage of members that CWNU 332 shares with each listed object.

Visualization

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