CWNU 3294

0.00 UTI

0.25

C_N

0.37

C_dens

0.75

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 25

Stellar density (N₅₀/rad) 1.9 [N/pc²]

C3 classification AB

C_N 0.25 Poorly populated
C_dens 0.37 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 3294 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate extinction. It is catalogued as a very young 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.

Very distant Moderate extinction Very young

Data

🔍 Search references for CWNU 3294 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–	359.49	63.793	0.167	-1.955	-0.525	-115.394
He et al.	2023	359.46	63.793	0.177	-1.972	-0.534	–

💡 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–	5.01	2.05	–	16	–	–	–	–
He et al.	2023	5.01	2.05	–	16	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 937	100.0	359.48	63.8	0.17	-1.95	-0.53	-115.39	0.29

💡 Note: The % column shows the percentage of members that CWNU 3294 shares with each listed object.

Visualization

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