CWNU 394

0.12 UTI

0.48

C_N

0.32

C_dens

0.5

C_C3

0.0

C_lit

0.46

C_dup

N₅₀ (P>50% members) 48

Stellar density (N₅₀/rad) 1.6 [N/pc²]

C3 classification BB

C_N 0.48 Poorly populated
C_dens 0.32 Loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.46 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 394 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, young cluster (see Parameters). It is rarely studied in the literature.

⚠️ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry, and a moderate percentage with at least one entry reported in the same catalogue. See table with shared members information.

Relatively close Moderate extinction Metal-rich Young

Data

🔍 Search references for CWNU 394 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–	348.155	57.483	0.917	0.25	-1.351	-27.344
He et al.	2022	348.051	57.538	0.913	0.225	-1.33	–
He et al.	2022	348.324	57.527	0.92	0.27	-1.37	-24.5

💡 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–	1.12	2.055	–	71	0.916	–	–	–
He et al.	2022	–	2.25	–	79	–	–	–	–
He et al.	2022	1.12	1.86	–	63	0.916	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 14366	100.0	348.22	57.48	0.92	0.24	-1.34	-29.86	0.02
LISC 3420	54.2	348.1	57.47	0.91	0.26	-1.37	-31.89	0.24
Theia 2526	52.1	348.12	57.48	0.91	0.27	-1.37	-31.89	0.0
CWNU 415	47.9	347.86	57.41	0.91	0.24	-1.38	-23.5	0.04
CWNU 83	20.8	347.51	57.0	0.91	0.19	-1.4	-19.28	0.05

💡 Note: The % column shows the percentage of members that CWNU 394 shares with each listed object.

Visualization

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