CWNU 4116

0.08 UTI

0.0

C_N

0.97

C_dens

0.25

C_C3

0.0

C_lit

0.32

C_dup

C3 classification CC

Number of members (P>50%) 24

Radius (P>50% members) 3.4 [arcmin]

C_N 0.0 Sparse
C_dens 0.97 Very dense
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.32 Possibly duplicate

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

Overview

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CWNU 4116 is a sparse, very dense object of low C3 quality. Its parallax locates it at a moderate distance, near 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 possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate extinction Very young

Data

🔍 Search references for CWNU 4116 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	–	82.499	33.436	0.446	0.211	-1.934	9.726
He et al.	2023	82.509	33.435	0.459	0.183	-1.943	29.87

💡 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	1.91	1.60	–	8	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
SAI 51	68.0	82.51	33.43	0.45	0.3	-1.95	9.56	0.38
Teutsch 133	4.0	82.48	33.52	0.31	-0.14	-1.59	13.37	0.13

💡 Note: The % column shows the percentage of members that CWNU 4116 shares with each listed object.

Visualization

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