CWWDL 14187

0.00 UTI

0.0

C_N

0.57

C_dens

0.75

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 24

Stellar density (N₅₀/rad) 2.9 [N/pc²]

C3 classification AB

C_N 0.0 Sparse
C_dens 0.57 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWWDL 14187 is a sparse, moderately dense object of high C3 quality. Its parallax locates it at a relatively close 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. See table with shared members information.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 14187 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–	185.361	-61.065	0.784	-7.045	-0.611	-12.925
Chi et al.	2023	185.417	-61.116	0.776	-7.002	-0.567	-11.211

💡 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–	–	–	–	66	0.200	–	–	–
Chi et al.	2023	–	–	–	66	0.200	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 252	100.0	185.37	-61.06	0.78	-7.07	-0.67	-20.39	0.56

💡 Note: The % column shows the percentage of members that CWWDL 14187 shares with each listed object.

Visualization

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