CWNU 3969

0.06 UTI

0.0

C_N

0.04

C_dens

0.38

C_C3

0.0

C_lit

0.72

C_dup

C3 classification CB

Number of members (P>50%) 20

Radius (P>50% members) 4.5 [arcmin]

C_N 0.0 Sparse
C_dens 0.04 Very loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.72 Likely unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWNU 3969 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by high extinction. It is catalogued as a very young cluster (see Parameters). It was recently reported in the literature.

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

Extremely distant High extinction Very young

Data

🔍 Search references for CWNU 3969 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	–	328.272	56.683	0.132	-2.75	-2.221	-10.736
He et al.	2023	328.272	56.683	0.148	-2.734	-2.217	-10.74

💡 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]	Bfr	BSS
He et al.	2023	10.47	4.95	–	2	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Teutsch 324	28.0	327.95	56.71	0.13	-2.85	-2.24	–	0.28

💡 Note: The % column shows the percentage of members that CWNU 3969 shares with each listed object.

Visualization

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