CWNU 3352

0.41 UTI

0.54

C_N

0.54

C_dens

1.0

C_C3

0.0

C_lit

1.0

C_dup

N_m (P>50%) 57

Core radius and density 1.6 [pc], 2.7 [pc^-2]

C3 classification AA

C_N 0.54 Moderately populated
C_dens 0.54 Moderately dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 3352 is a moderately populated, moderately dense object of very high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by high extinction. It is catalogued as an old cluster (see Parameters). It was recently reported in the literature.

Distant High extinction Old

Data

🔍 Search references for CWNU 3352 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–	242.387	-54.697	0.184	-3.107	-3.746	-87.87
He et al.	2023	242.381	-54.699	0.167	-3.131	-3.742	-87.87

💡 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–	4.17	3.35	–	2512	–	–	–	–
He et al.	2023	4.17	3.35	–	2512	–	–	–	–

Visualization

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