CWNU 184

0.00 UTI

0.57

C_N

0.88

C_dens

0.75

C_C3

0.0

C_lit

0.0

C_dup

C3 classification AB

Number of members (P>50%) 65

Radius (P>50% members) 8.5 [arcmin]

C_N 0.57 Moderately populated
C_dens 0.88 Dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

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

Overview

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CWNU 184 is a moderately populated, dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

⚠️ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate extinction Metal-rich Intermediate age

Data

🔍 Search references for CWNU 184 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	–	146.866	-50.561	0.642	-7.143	5.006	13.245
He et al.	2022	146.865	-50.586	0.64	-7.14	5.0	43.7

💡 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	2.00	1.56	–	316	0.968	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1465	100.0	146.89	-50.57	0.64	-7.15	5.0	20.53	0.49
Theia 6111	95.4	146.9	-50.57	0.64	-7.15	5.0	18.59	0.0
CWWDL 14184	86.2	146.87	-50.55	0.65	-7.14	5.01	18.79	0.0
CWWDL 13969	61.5	146.87	-50.54	0.64	-7.15	5.03	20.92	0.0

💡 Note: The % column shows the percentage of members that CWNU 184 shares with each listed object.

Visualization

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