CKCWDM 46470

0.05 UTI

0.0

C_N

0.08

C_dens

0.25

C_C3

0.0

C_lit

0.76

C_dup

N₅₀ (P>50% members) 19

Stellar density (N₅₀/rad) 0.4 [N/pc²]

C3 classification CC

C_N 0.0 Sparse
C_dens 0.08 Very loose
C_C3 0.25 Low 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

ℹ️

CKCWDM 46470 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, 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, and a significant percentage with at least one entry reported in the same catalogue. 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 Moderate extinction Metal-poor Intermediate age

Data

🔍 Search references for CKCWDM 46470 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	122.467	-32.206	0.191	-2.256	2.983	69.183
Chi et al.	2025	122.479	-32.279	0.2	-2.23	2.954	–

💡 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–	5.01	2.86	–	816	-0.857	–	–	–
Chi et al.	2025	5.01	2.86	–	816	-0.857	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CKCWDM 46404	72.0	122.47	-32.2	0.17	-2.27	2.99	98.94	0.03
CWNU 2588	24.0	122.27	-32.19	0.24	-2.3	3.04	88.75	0.16

💡 Note: The % column shows the percentage of members that CKCWDM 46470 shares with each listed object.

Visualization

ℹ️