CWWDL 14526

0.00 UTI

0.47

C_N

0.49

C_dens

0.75

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 47

Stellar density (N₅₀/rad) 2.5 [N/pc²]

C3 classification BA

C_N 0.47 Poorly populated
C_dens 0.49 Loose
C_C3 0.75 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 14526 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a close distance, below 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 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 Very young

Data

🔍 Search references for CWWDL 14526 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–	314.199	-6.688	1.75	5.114	1.958	-15.954
Chi et al.	2023	314.171	-6.695	1.772	5.114	1.965	-20.991

💡 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	0.070	–	–	–
Chi et al.	2023	–	–	–	6	0.070	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UPK 51	100.0	314.12	-6.69	1.75	5.08	1.94	-16.05	0.72

💡 Note: The % column shows the percentage of members that CWWDL 14526 shares with each listed object.

Visualization

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