CWWDL 13331

0.00 UTI

0.49

C_N

1.0

C_dens

0.38

C_C3

0.0

C_lit

0.0

C_dup

C3 classification CB

Number of members (P>50%) 49

Radius (P>50% members) 6.4 [arcmin]

C_N 0.49 Poorly populated
C_dens 1.0 Very dense
C_C3 0.38 Low 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 13331 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a relatively 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 13331 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	–	125.537	-42.122	0.662	-4.31	5.28	-7.141
Chi et al.	2023	125.575	-42.154	0.666	-4.329	5.214	78.933

💡 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	–	–	–	1	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Majaess 99	100.0	125.54	-42.1	0.66	-4.34	5.25	0.76	0.6
OC 0463	71.4	125.49	-42.1	0.66	-4.32	5.2	0.76	0.0
OC 0466	59.2	125.65	-42.12	0.66	-4.31	5.31	0.76	0.01

💡 Note: The % column shows the percentage of members that CWWDL 13331 shares with each listed object.

Visualization

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