CWNU 3379

0.36 UTI

0.79

C_N

0.48

C_dens

0.75

C_C3

0.0

C_lit

0.88

C_dup

N₅₀ (P>50% members) 207

Stellar density (N₅₀/rad) 2.4 [N/pc²]

C3 classification AB

C_N 0.79 Rich
C_dens 0.48 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.88 Very likely unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 3379 is a rich, loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a young cluster (see Parameters). It was recently reported in the literature.

Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.

Distant High extinction Young

Data

🔍 Search references for CWNU 3379 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–	334.589	59.086	0.251	-3.437	-2.446	-74.474
He et al.	2023	334.589	59.1	0.251	-3.44	-2.44	-143.42

💡 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–	3.09	3.45	–	32	–	–	–	–
He et al.	2023	3.09	3.45	–	32	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FSR 0366	12.1	334.56	59.06	0.25	-3.43	-2.44	–	0.28

💡 Note: The % column shows the percentage of members that CWNU 3379 shares with each listed object.

Visualization

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