CWNU 3290

0.04 UTI

0.43

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.09

C_dup

N₅₀ (P>50% members) 43

Stellar density (N₅₀/rad) 6.4 [N/pc²]

C3 classification BA

C_N 0.43 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.09 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 3290 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a large 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 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.

Distant Moderate extinction Intermediate age

Data

🔍 Search references for CWNU 3290 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–	90.253	32.009	0.169	0.928	-1.116	10.936
He et al.	2023	90.253	32.009	0.187	0.917	-1.103	10.94

💡 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–	4.68	2.4	–	251	–	–	–	–
He et al.	2023	4.68	2.40	–	251	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1413	90.7	90.26	32.01	0.18	0.91	-1.1	10.94	0.49

💡 Note: The % column shows the percentage of members that CWNU 3290 shares with each listed object.

Visualization

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