CWWDL 14581

0.00 UTI

0.47

C_N

0.95

C_dens

0.75

C_C3

0.0

C_lit

0.0

C_dup

C3 classification BA

Number of members (P>50%) 47

Radius (P>50% members) 23.7 [arcmin]

C_N 0.47 Poorly populated
C_dens 0.95 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

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

Overview

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CWWDL 14581 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by low extinction. 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.

Close Low extinction Near-solar metallicity Young

Data

🔍 Search references for CWWDL 14581 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	–	12.157	50.127	2.192	7.366	-3.129	-5.551
Wei et al.	2025	12.306	50.382	2.213	7.389	-3.095	–
Chi et al.	2023	12.22	49.999	2.185	7.405	-3.107	-9.829

💡 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
Wei et al.	2025	0.58	0.75	–	50	-0.250	226	0.25	–
Chi et al.	2023	–	–	–	9	0.420	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
LISC 3534	100.0	12.19	50.25	2.18	7.37	-3.08	-5.55	0.72

💡 Note: The % column shows the percentage of members that CWWDL 14581 shares with each listed object.

Visualization

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