CWWDL 13441

0.00 UTI

0.0

C_N

0.48

C_dens

0.75

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 20

Stellar density (N₅₀/rad) 2.4 [N/pc²]

C3 classification BA

C_N 0.0 Sparse
C_dens 0.48 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWWDL 13441 is a sparse, loose object of high C3 quality. Its parallax locates it at a moderate distance, near 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 13441 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	99999–	255.28	-44.672	0.445	-1.095	-2.805	-33.627
Chi et al.	2023	255.518	-44.712	0.446	-1.109	-2.776	-33.884

💡 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]	B_frac	BSS
UCC	99999–	–	–	–	19	0.440	–	–	–
Chi et al.	2023	–	–	–	19	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Melotte 158	100.0	255.19	-44.68	0.42	-1.04	-2.89	-34.4	1.0
OC 0672	8.0	255.19	-44.68	0.46	-1.06	-2.92	-33.95	0.0

💡 Note: The % column shows the percentage of members that CWWDL 13441 shares with each listed object.

Visualization

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