CKCWDM 54944

0.06 UTI

0.63

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.12

C_dup

N₅₀ (P>50% members) 76

Stellar density (N₅₀/rad) 5.9 [N/pc²]

C3 classification AB

C_N 0.63 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.12 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CKCWDM 54944 is a moderately populated, very dense object of high 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.

⚠️ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Very distant Moderate extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for CKCWDM 54944 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–	127.017	-34.056	0.178	-3.312	4.185	72.737
Chi et al.	2025	127.018	-34.08	0.165	-3.324	4.244	–

💡 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–	6.08	1.88	–	765	0.302	–	–	–
Chi et al.	2025	6.08	1.88	–	765	0.302	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 1280	88.2	127.02	-34.05	0.18	-3.32	4.18	73.43	0.54

💡 Note: The % column shows the percentage of members that CKCWDM 54944 shares with each listed object.

Visualization

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