CWNU 4114

0.27 UTI

0.64

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.57

C_dup

N₅₀ (P>50% members) 77

Stellar density (N₅₀/rad) 6.8 [N/pc²]

C3 classification AB

C_N 0.64 Moderately populated
C_dens 1.0 Very 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 4114 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as an intermediate-age 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 High extinction Intermediate age

Data

🔍 Search references for CWNU 4114 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–	202.503	-62.494	0.242	-6.019	-1.737	-53.163
He et al.	2023	202.489	-62.488	0.231	-6.031	-1.729	-53.74

💡 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]	B_frac	BSS
UCC	99999–	3.39	4.7	–	398	–	–	–	–
He et al.	2023	3.39	4.70	–	398	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2592	42.9	202.47	-62.5	0.24	-6.02	-1.74	-53.74	0.37

💡 Note: The % column shows the percentage of members that CWNU 4114 shares with each listed object.

Visualization

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