CKCWDM 48869

0.05 UTI

0.62

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.11

C_dup

N₅₀ (P>50% members) 73

Stellar density (N₅₀/rad) 5.2 [N/pc²]

C3 classification AB

C_N 0.62 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.11 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CKCWDM 48869 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 high 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 High extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for CKCWDM 48869 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–	175.976	-60.526	0.178	-7.872	1.765	-4.187
Chi et al.	2025	175.947	-60.533	0.188	-7.841	1.75	–

💡 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–	5.31	4.92	–	814	-0.274	–	–	–
Chi et al.	2025	5.31	4.92	–	814	-0.274	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1505	89.0	175.99	-60.53	0.17	-7.88	1.77	2.8	0.62
HSC 2450	20.5	175.96	-60.51	0.27	-7.91	1.78	–	0.07

💡 Note: The % column shows the percentage of members that CKCWDM 48869 shares with each listed object.

Visualization

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