CWWDL 13332

0.01 UTI

0.0

C_N

0.49

C_dens

0.75

C_C3

0.0

C_lit

0.04

C_dup

C3 classification AB

Number of members (P>50%) 23

Radius (P>50% members) 5.7 [arcmin]

C_N 0.0 Sparse
C_dens 0.49 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.04 Very likely duplicate

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

Overview

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CWWDL 13332 is a sparse, loose object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane. It is catalogued as a metal-poor, 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.

Metal-poor Very young

Data

🔍 Search references for CWWDL 13332 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	–	129.656	-46.256	0.541	-5.784	5.127	-9.58
Chi et al.	2023	129.432	-46.241	0.538	-5.741	5.133	43.289

💡 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	–	–	–	5	-0.880	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0481	96.0	129.65	-46.22	0.54	-5.81	5.15	-9.58	0.19
Pismis 6	64.0	129.83	-46.25	0.54	-5.87	5.11	17.73	0.96
FoF 58	52.0	129.9	-46.29	0.54	-5.83	5.09	-1.51	0.14

💡 Note: The % column shows the percentage of members that CWWDL 13332 shares with each listed object.

Visualization

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