CWWDL 3524

0.03 UTI

0.74

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.05

C_dup

C3 classification AB

Number of members (P>50%) 97

Radius (P>50% members) 3.8 [arcmin]

C_N 0.74 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.05 Very likely duplicate

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

Overview

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CWWDL 3524 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate 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 3524 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	–	109.851	-21.422	0.34	-1.895	2.53	81.639
Chi et al.	2023	109.858	-21.427	0.337	-1.941	2.544	56.692

💡 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
Chi et al.	2023	–	–	–	10	0.070	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
LISC 1024	94.8	109.85	-21.42	0.34	-1.89	2.55	63.81	0.12
UBC 457	89.7	109.85	-21.41	0.34	-1.88	2.51	49.83	0.65

💡 Note: The % column shows the percentage of members that CWWDL 3524 shares with each listed object.

Visualization

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