CWWDL 14223

0.00 UTI

0.41

C_N

0.83

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

C3 classification AA

Number of members (P>50%) 41

Radius (P>50% members) 6.8 [arcmin]

C_N 0.41 Poorly populated
C_dens 0.83 Dense
C_C3 1.0 Very 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 14223 is a poorly populated, dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane. It is catalogued as a metal-poor, intermediate-age 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.

Metal-poor Intermediate age

Data

🔍 Search references for CWWDL 14223 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	–	191.943	-59.372	0.629	-5.933	-0.282	-19.789
Chi et al.	2023	191.9	-59.358	0.657	-5.941	-0.299	-21.725

💡 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	–	–	–	107	-0.880	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 290	100.0	191.89	-59.37	0.61	-5.93	-0.25	-23.5	0.78
CWWDL 14045	56.1	191.79	-59.39	0.61	-5.96	-0.23	-23.55	0.0

💡 Note: The % column shows the percentage of members that CWWDL 14223 shares with each listed object.

Visualization

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