CWNU 84

0.18 UTI

0.52

C_N

0.94

C_dens

0.75

C_C3

0.0

C_lit

0.41

C_dup

C3 classification AB

Number of members (P>50%) 54

Radius (P>50% members) 5.1 [arcmin]

C_N 0.52 Moderately populated
C_dens 0.94 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.41 Possibly duplicate

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

Overview

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CWNU 84 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by low extinction. It is catalogued as a metal-rich, intermediate-age cluster (see Parameters). It is rarely studied 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 Low extinction Metal-rich Intermediate age

Data

🔍 Search references for CWNU 84 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	–	159.116	-65.181	0.437	-5.758	2.626	-17.085
He et al.	2022	159.093	-65.174	0.44	-5.76	2.65	–

💡 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.	2022	2.04	0.72	–	251	0.862	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1494	59.3	159.09	-65.19	0.44	-5.76	2.63	-17.42	0.45

💡 Note: The % column shows the percentage of members that CWNU 84 shares with each listed object.

Visualization

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