CWWDL 14443

0.00 UTI

0.38

C_N

1.0

C_dens

0.5

C_C3

0.0

C_lit

0.0

C_dup

C3 classification BB

Number of members (P>50%) 38

Radius (P>50% members) 11.8 [arcmin]

C_N 0.38 Poorly populated
C_dens 1.0 Very dense
C_C3 0.5 Intermediate 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 14443 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a close^* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, 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, and a moderate percentage with at least one entry reported in the same catalogue. See table with shared members information.

(*): The parallax distance estimate (~0.60 kpc) differs significantly from the median photometric distance (~1.07 kpc).

Relatively close Moderate extinction Near-solar metallicity Young

Data

🔍 Search references for CWWDL 14443 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	–	288.498	14.275	1.664	2.437	0.989	-5.638
Wei et al.	2025	288.529	14.321	1.683	2.443	1.027	–
Chi et al.	2023	288.529	14.365	1.666	2.426	0.901	-6.452

💡 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
Wei et al.	2025	1.07	1.81	–	174	-0.250	283	0.35	–
Chi et al.	2023	–	–	–	6	-0.180	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UPK 53	100.0	288.52	14.37	1.68	2.45	1.02	-5.7	0.79
CWWDL 14632	44.7	288.6	14.35	1.69	2.42	1.06	-6.7	0.0

💡 Note: The % column shows the percentage of members that CWWDL 14443 shares with each listed object.

Visualization

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