CWWDL 14466

0.01 UTI

0.57

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.03

C_dup

C3 classification AB

Number of members (P>50%) 64

Radius (P>50% members) 7.2 [arcmin]

C_N 0.57 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.03 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWWDL 14466 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a close distance, above the mid-plane. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

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

Near-solar metallicity Intermediate age

Data

🔍 Search references for CWWDL 14466 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	–	192.972	-57.373	1.064	-12.961	-4.572	-2.684
Chi et al.	2023	193.009	-57.393	1.065	-13.028	-4.601	-3.446

💡 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]	Bfr	BSS
Chi et al.	2023	–	–	–	123	-0.180	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UPK 578	96.9	192.97	-57.37	1.06	-12.96	-4.57	-2.68	0.78

💡 Note: The % column shows the percentage of members that CWWDL 14466 shares with each listed object.

Visualization

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