CWWDL 14020

0.03 UTI

0.38

C_N

0.81

C_dens

0.75

C_C3

0.0

C_lit

0.08

C_dup

N₅₀ (P>50% members) 38

Stellar density (N₅₀/rad) 4.0 [N/pc²]

C3 classification AB

C_N 0.38 Poorly populated
C_dens 0.81 Dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.08 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWWDL 14020 is a poorly populated, dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. 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, and a large percentage with at least one entry reported in the same catalogue. See table with shared members information.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 14020 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–	298.299	32.633	0.465	-2.462	-3.45	10.049
Chi et al.	2023	298.266	32.558	0.452	-2.456	-3.501	-12.626

💡 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–	–	–	–	81	0.200	–	–	–
Chi et al.	2023	–	–	–	81	0.200	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 11597	94.7	298.3	32.65	0.47	-2.46	-3.46	-1.29	0.06
HXHWL 46	92.1	298.31	32.65	0.47	-2.48	-3.44	10.05	0.56
UBC 1079	73.7	298.32	32.66	0.48	-2.48	-3.45	10.05	0.02

💡 Note: The % column shows the percentage of members that CWWDL 14020 shares with each listed object.

Visualization

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