CWWDL 14576

0.00 UTI

0.0

C_N

0.33

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 24

Stellar density (N₅₀/rad) 1.6 [N/pc²]

C3 classification AA

C_N 0.0 Sparse
C_dens 0.33 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 14576 is a sparse, loose object of very high C3 quality. Its parallax locates it at a very 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 14576 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–	116.755	-47.369	2.516	-4.685	8.885	20.471
Chi et al.	2023	116.195	-47.588	2.528	-4.68	8.844	20.795

💡 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–	–	–	–	1	0.420	–	–	–
Chi et al.	2023	–	–	–	1	0.420	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FoF 2387	100.0	117.39	-46.67	2.53	-4.71	8.96	17.63	0.52
OCSN 200	100.0	117.36	-46.54	2.54	-4.69	9.01	17.63	0.04
CWWL 3526	12.0	117.91	-46.81	2.54	-4.78	8.82	19.74	0.0
OC 0470	4.0	117.34	-46.37	2.55	-4.71	9.06	17.63	0.66

💡 Note: The % column shows the percentage of members that CWWDL 14576 shares with each listed object.

Visualization

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