CWWDL 14391

0.12 UTI

0.42

C_N

1.0

C_dens

0.5

C_C3

0.0

C_lit

0.31

C_dup

C3 classification BB

Number of members (P>50%) 42

Radius (P>50% members) 5.3 [arcmin]

C_N 0.42 Poorly populated
C_dens 1.0 Very dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.31 Possibly duplicate

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

Overview

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CWWDL 14391 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane. It is catalogued as a metal-poor, 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.

Metal-poor Young

Data

🔍 Search references for CWWDL 14391 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	–	255.596	-42.879	0.932	0.486	-2.447	5.051
Chi et al.	2023	255.616	-42.888	0.926	0.458	-2.414	4.182

💡 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	–	–	–	58	-0.580	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 2341	100.0	255.6	-42.89	0.93	0.49	-2.45	5.05	0.03
CWNU 285	69.0	255.63	-42.88	0.93	0.49	-2.48	5.8	0.36

💡 Note: The % column shows the percentage of members that CWWDL 14391 shares with each listed object.

Visualization

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