CWNU 33

0.03 UTI

0.28

C_N

0.73

C_dens

0.75

C_C3

0.0

C_lit

0.07

C_dup

C3 classification AB

Number of members (P>50%) 28

Radius (P>50% members) 7.0 [arcmin]

C_N 0.28 Poorly populated
C_dens 0.73 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.07 Very likely duplicate

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

Overview

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CWNU 33 is a poorly populated, moderately 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 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.

Relatively close Moderate extinction Metal-rich Intermediate age

Data

🔍 Search references for CWNU 33 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	–	75.636	19.687	0.736	0.48	-3.61	-13.516
He et al.	2022	75.639	19.688	0.75	0.47	-3.6	–

💡 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	1.48	1.50	–	631	0.862	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0298	92.9	75.63	19.72	0.73	0.47	-3.61	-13.52	0.49

💡 Note: The % column shows the percentage of members that CWNU 33 shares with each listed object.

Visualization

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