CKCWDM 58488

0.16 UTI

0.38

C_N

0.08

C_dens

0.38

C_C3

0.0

C_lit

0.97

C_dup

N₅₀ (P>50% members) 38

Stellar density (N₅₀/rad) 0.4 [N/pc²]

C3 classification BC

C_N 0.38 Poorly populated
C_dens 0.08 Very loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.97 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CKCWDM 58488 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate 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 a unique object, which shares a very 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=0.97) 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 58488 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–	0.732	64.414	0.224	-2.324	-0.693	-45.076
Chi et al.	2025	0.691	64.437	0.198	-2.357	-0.663	–

💡 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–	5.04	4.5	–	777	0.253	–	–	–
Chi et al.	2025	5.04	4.50	–	777	0.253	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 11749	2.6	1.3	64.41	0.26	-2.31	-0.84	-24.01	0.05

💡 Note: The % column shows the percentage of members that CKCWDM 58488 shares with each listed object.

Visualization

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