CWWDL 14085

0.03 UTI

0.0

C_N

0.32

C_dens

0.38

C_C3

0.0

C_lit

0.24

C_dup

C3 classification BC

Number of members (P>50%) 23

Radius (P>50% members) 5.9 [arcmin]

C_N 0.0 Sparse
C_dens 0.32 Loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.24 Likely duplicate

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

Overview

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CWWDL 14085 is a sparse, loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. It is catalogued as a metal-poor, young cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is 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 Young

Data

🔍 Search references for CWWDL 14085 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	–	109.991	3.226	0.455	-1.996	-0.307	62.721
Chi et al.	2023	109.992	3.224	0.455	-2.03	-0.189	64.993

💡 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	–	–	–	87	-0.580	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 1331	76.0	110.0	3.26	0.46	-1.99	-0.32	62.72	0.39

💡 Note: The % column shows the percentage of members that CWWDL 14085 shares with each listed object.

Visualization

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