CWWDL 14372

0.02 UTI

0.36

C_N

0.72

C_dens

0.5

C_C3

0.0

C_lit

0.06

C_dup

N₅₀ (P>50% members) 36

Stellar density (N₅₀/rad) 3.6 [N/pc²]

C3 classification BB

C_N 0.36 Poorly populated
C_dens 0.72 Moderately dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.06 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWWDL 14372 is a poorly populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane. It is catalogued as a near-solar metallicity, very 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.

Near-solar metallicity Very young

Data

🔍 Search references for CWWDL 14372 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	99999–	69.515	42.981	0.966	0.14	-2.536	15.848
Chi et al.	2023	69.536	43.046	0.959	0.184	-2.548	10.248

💡 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]	B_frac	BSS
UCC	99999–	–	–	–	9	0.200	–	–	–
Chi et al.	2023	–	–	–	9	0.200	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
COIN-Gaia 39	94.4	69.52	42.97	0.97	0.14	-2.52	13.51	0.57

💡 Note: The % column shows the percentage of members that CWWDL 14372 shares with each listed object.

Visualization

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