CWNU 3967

0.21 UTI

0.37

C_N

0.76

C_dens

0.75

C_C3

0.0

C_lit

0.57

C_dup

N₅₀ (P>50% members) 37

Stellar density (N₅₀/rad) 3.8 [N/pc²]

C3 classification AB

C_N 0.37 Poorly populated
C_dens 0.76 Dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.57 Likely unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 3967 is a poorly populated, dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very 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.

Distant Very high extinction Very young

Data

🔍 Search references for CWNU 3967 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–	270.737	-22.815	0.262	-0.967	-2.379	41.247
He et al.	2023	270.724	-22.815	0.274	-0.964	-2.376	843.71

💡 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–	3.8	5.95	–	3	–	–	–	–
He et al.	2023	3.80	5.95	–	3	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Teutsch 72	43.2	270.71	-22.81	0.31	-1.07	-2.52	63.25	0.39

💡 Note: The % column shows the percentage of members that CWNU 3967 shares with each listed object.

Visualization

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