CWWDL 13341

0.11 UTI

0.37

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.27

C_dup

C3 classification AB

Number of members (P>50%) 37

Radius (P>50% members) 2.7 [arcmin]

C_N 0.37 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.27 Possibly duplicate

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

Overview

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CWWDL 13341 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 13341 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	–	235.004	-58.48	0.565	-2.174	-3.539	–
Chi et al.	2023	235.02	-58.49	0.554	-2.192	-3.545	–

💡 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	–	–	–	29	0.320	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 2227	97.3	235.0	-58.49	0.57	-2.17	-3.55	–	0.1
HXHWL 67	73.0	235.0	-58.49	0.56	-2.16	-3.53	–	0.41

💡 Note: The % column shows the percentage of members that CWWDL 13341 shares with each listed object.

Visualization

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