CWWDL 14664

0.18 UTI

0.66

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.33

C_dup

N₅₀ (P>50% members) 81

Stellar density (N₅₀/rad) 5.8 [N/pc²]

C3 classification AA

C_N 0.66 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.33 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWWDL 14664 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a close distance, above the mid-plane. It is catalogued as a near-solar metallicity, very young 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.

Near-solar metallicity Very young

Data

🔍 Search references for CWWDL 14664 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–	270.356	3.031	1.795	0.639	-8.882	-7.342
Chi et al.	2023	270.361	2.986	1.785	0.609	-8.921	-8.166

💡 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–	–	–	–	4	-0.100	–	–	–
Chi et al.	2023	–	–	–	4	-0.100	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Melotte 186	66.7	270.41	3.16	1.79	0.65	-8.83	-7.42	0.92
HSC 297	4.9	270.7	2.76	1.94	0.42	-8.66	-4.84	0.12

💡 Note: The % column shows the percentage of members that CWWDL 14664 shares with each listed object.

Visualization

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