CKCWDM 14529

0.12 UTI

0.0

C_N

0.01

C_dens

0.75

C_C3

0.0

C_lit

0.76

C_dup

N₅₀ (P>50% members) 17

Stellar density (N₅₀/rad) 0.1 [N/pc²]

C3 classification AB

C_N 0.0 Sparse
C_dens 0.01 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.76 Very likely unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CKCWDM 14529 is a sparse, very loose object of high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=0.76) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Very distant High extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for CKCWDM 14529 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–	20.293	64.718	0.136	-1.194	0.088	-56.417
Chi et al.	2025	20.246	64.862	0.13	-1.192	0.087	–

💡 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–	7.7	3.96	–	773	0.318	–	–	–
Chi et al.	2025	7.70	3.96	–	773	0.318	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 600	24.0	20.77	64.57	0.17	-1.18	0.09	-58.49	0.46

💡 Note: The % column shows the percentage of members that CKCWDM 14529 shares with each listed object.

Visualization

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