CWNU 3326

0.01 UTI

0.0

C_N

0.18

C_dens

0.38

C_C3

0.0

C_lit

0.12

C_dup

C3 classification BC

Number of members (P>50%) 24

Radius (P>50% members) 14.5 [arcmin]

C_N 0.0 Sparse
C_dens 0.18 Very loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.12 Likely duplicate

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

Overview

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CWNU 3326 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close 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.

Relatively close Moderate extinction Intermediate age

Data

🔍 Search references for CWNU 3326 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	–	349.63	66.545	0.819	0.195	-2.053	-14.519
He et al.	2023	349.838	66.43	0.819	0.177	-2.053	-10.36

💡 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	1.29	2.50	–	794	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 912	88.0	349.63	66.61	0.82	0.2	-2.05	-14.52	0.24

💡 Note: The % column shows the percentage of members that CWNU 3326 shares with each listed object.

Visualization

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