CWWDL 14382

0.00 UTI

0.3

C_N

1.0

C_dens

0.25

C_C3

0.0

C_lit

0.0

C_dup

C3 classification DB

Number of members (P>50%) 30

Radius (P>50% members) 7.2 [arcmin]

C_N 0.3 Poorly populated
C_dens 1.0 Very dense
C_C3 0.25 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 14382 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 14382 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	–	124.33	-37.81	1.444	-8.09	5.692	31.742
Wei et al.	2025	124.35	-37.937	1.393	-7.988	5.758	–
Chi et al.	2023	124.31	-37.834	1.444	-8.021	5.691	33.01

💡 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	0.92	0.43	–	32	0.500	214	0.51	–
Chi et al.	2023	–	–	–	9	0.160	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UPK 502	100.0	124.36	-37.77	1.43	-8.08	5.67	31.9	0.77

💡 Note: The % column shows the percentage of members that CWWDL 14382 shares with each listed object.

Visualization

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