CWWDL 14565

0.00 UTI

0.25

C_N

0.27

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 25

Stellar density (N₅₀/rad) 1.3 [N/pc²]

C3 classification AA

C_N 0.25 Poorly populated
C_dens 0.27 Loose
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWWDL 14565 is a poorly populated, loose object of very high C3 quality. Its parallax locates it at a close distance, below the mid-plane. It is catalogued as a near-solar metallicity, young 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 Young

Data

🔍 Search references for CWWDL 14565 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–	5.587	46.515	1.783	-6.392	-5.103	-16.394
Chi et al.	2023	5.721	46.523	1.769	-6.321	-5.095	-15.58

💡 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–	–	–	–	50	0.370	–	–	–
Chi et al.	2023	–	–	–	50	0.370	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Alessi 94	100.0	5.38	46.54	1.78	-6.41	-5.09	-15.84	0.63

💡 Note: The % column shows the percentage of members that CWWDL 14565 shares with each listed object.

Visualization

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