CWNU 3348

0.01 UTI

0.31

C_N

0.11

C_dens

0.38

C_C3

0.0

C_lit

0.06

C_dup

N_m (P>50%) 31

Core radius and density 2.2 [pc], 0.5 [pc^-2]

C3 classification CB

C_N 0.31 Poorly populated
C_dens 0.11 Very loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.06 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 3348 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, near 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.

Relatively close Moderate extinction Intermediate age

Data

🔍 Search references for CWNU 3348 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–	2.524	61.369	0.649	-1.141	-2.458	3.048
He et al.	2023	2.521	61.369	0.649	-1.155	-2.458	-40.48

💡 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–	1.62	2.05	–	200	–	–	–	–
He et al.	2023	1.62	2.05	–	200	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 941	93.5	2.55	61.36	0.64	-1.13	-2.46	3.05	0.17

💡 Note: The % column shows the percentage of members that CWNU 3348 shares with each listed object.

Visualization

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