CWWDL 14643

0.00 UTI

0.27

C_N

1.0

C_dens

0.38

C_C3

0.0

C_lit

0.0

C_dup

C3 classification CB

Number of members (P>50%) 27

Radius (P>50% members) 13.0 [arcmin]

C_N 0.27 Poorly populated
C_dens 1.0 Very dense
C_C3 0.38 Low 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 14643 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. 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. See table with shared members information.

Close Low extinction Near-solar metallicity Young

Data

🔍 Search references for CWWDL 14643 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	–	268.067	-27.035	1.677	0.878	-5.168	-0.84
Wei et al.	2025	268.106	-26.974	1.664	0.898	-5.137	–
Chi et al.	2023	268.088	-27.012	1.726	0.895	-5.165	-0.909

💡 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
Wei et al.	2025	0.71	0.78	–	83	0.000	225	0.44	–
Chi et al.	2023	–	–	–	3	0.160	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HXHWL 29	100.0	268.07	-27.02	1.66	0.88	-5.12	0.19	0.63

💡 Note: The % column shows the percentage of members that CWWDL 14643 shares with each listed object.

Visualization

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