CKCWDM 13202

0.12 UTI

0.57

C_N

0.73

C_dens

0.75

C_C3

0.0

C_lit

0.28

C_dup

N₅₀ (P>50% members) 64

Stellar density (N₅₀/rad) 3.6 [N/pc²]

C3 classification AB

C_N 0.57 Moderately populated
C_dens 0.73 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.28 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CKCWDM 13202 is a moderately populated, moderately 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 possibly a duplicate object, which shares a significant 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 13202 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–	101.459	7.665	0.167	0.487	0.323	59.891
Chi et al.	2025	101.469	7.66	0.161	0.489	0.15	–

💡 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–	6.19	1.9	–	743	0.300	–	–	–
Chi et al.	2025	6.19	1.90	–	743	0.300	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1329	71.9	101.45	7.67	0.16	0.49	0.34	59.89	0.52

💡 Note: The % column shows the percentage of members that CKCWDM 13202 shares with each listed object.

Visualization

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