CWWDL 14184

0.00 UTI

0.54

C_N

0.81

C_dens

0.75

C_C3

0.0

C_lit

0.0

C_dup

C3 classification AB

Number of members (P>50%) 58

Radius (P>50% members) 8.4 [arcmin]

C_N 0.54 Moderately populated
C_dens 0.81 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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CWWDL 14184 is a moderately populated, dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported 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, and a significant percentage with at least one entry reported in the same catalogue. See table with shared members information.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 14184 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	–	146.867	-50.548	0.647	-7.141	5.008	18.79
Chi et al.	2023	146.858	-50.57	0.654	-7.13	5.015	11.941

💡 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
Chi et al.	2023	–	–	–	29	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 6111	100.0	146.9	-50.57	0.64	-7.15	5.0	18.59	0.0
UBC 1465	100.0	146.89	-50.57	0.64	-7.15	5.0	20.53	0.49
CWNU 184	96.6	146.87	-50.56	0.64	-7.14	5.01	13.24	0.0
CWWDL 13969	67.2	146.87	-50.54	0.64	-7.15	5.03	20.92	0.0

💡 Note: The % column shows the percentage of members that CWWDL 14184 shares with each listed object.

Visualization

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