CKCWDM 54095

0.02 UTI

0.0

C_N

0.05

C_dens

0.12

C_C3

0.0

C_lit

0.6

C_dup

N₅₀ (P>50% members) 17

Stellar density (N₅₀/rad) 0.2 [N/pc²]

C3 classification DC

C_N 0.0 Sparse
C_dens 0.05 Very loose
C_C3 0.12 Very low quality
C_lit 0.0 Rarely studied
C_dup 0.6 Likely unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CKCWDM 54095 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry, and a small percentage with at least one entry reported in the same catalogue. See table with shared members information.

Very distant Moderate extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for CKCWDM 54095 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–	110.173	-9.856	0.165	-1.159	1.127	79.973
Chi et al.	2025	110.206	-9.802	0.174	-1.122	1.152	–

💡 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–	5.74	1.38	–	777	0.331	–	–	–
Chi et al.	2025	5.74	1.38	–	777	0.331	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FoF 1408	40.0	110.08	-9.92	0.2	-1.17	0.99	65.45	0.17
CKCWDM 53972	20.0	110.07	-9.93	0.15	-1.06	0.97	66.76	0.01

💡 Note: The % column shows the percentage of members that CKCWDM 54095 shares with each listed object.

Visualization

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