CWNU 3351

0.05 UTI

0.45

C_N

0.18

C_dens

0.38

C_C3

0.0

C_lit

0.24

C_dup

N₅₀ (P>50% members) 45

Stellar density (N₅₀/rad) 0.9 [N/pc²]

C3 classification CB

C_N 0.45 Poorly populated
C_dens 0.18 Very loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.24 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 3351 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a young 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.

Distant Moderate extinction Young

Data

🔍 Search references for CWNU 3351 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–	115.073	-33.57	0.257	-2.247	3.044	–
He et al.	2023	115.091	-33.557	0.255	-2.245	3.062	68.87

💡 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–	3.02	2.05	–	50	–	–	–	–
He et al.	2023	3.02	2.05	–	50	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Bochum 15	75.6	115.08	-33.57	0.26	-2.24	3.04	–	0.3
Cmg 1050	26.7	114.86	-33.65	0.26	-2.24	3.03	–	0.06

💡 Note: The % column shows the percentage of members that CWNU 3351 shares with each listed object.

Visualization

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