CWWDL 14423

0.01 UTI

0.34

C_N

0.81

C_dens

0.75

C_C3

0.0

C_lit

0.03

C_dup

C3 classification AB

Number of members (P>50%) 34

Radius (P>50% members) 10.0 [arcmin]

C_N 0.34 Poorly populated
C_dens 0.81 Dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.03 Very likely duplicate

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

Overview

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CWWDL 14423 is a poorly populated, dense object of high C3 quality. Its parallax locates it at a close distance, above the mid-plane. It is catalogued as a metal-poor, 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. See table with shared members information.

Metal-poor Young

Data

🔍 Search references for CWWDL 14423 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	–	122.409	-27.15	1.006	-3.956	2.029	8.572
Chi et al.	2023	122.412	-27.133	1.002	-3.972	2.017	6.881

💡 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	–	–	–	33	-0.580	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HXHWL 65	97.1	122.41	-27.15	1.01	-3.96	2.03	8.09	0.52

💡 Note: The % column shows the percentage of members that CWWDL 14423 shares with each listed object.

Visualization

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