CWWDL 10428

0.08 UTI

0.0

C_N

0.02

C_dens

0.38

C_C3

0.0

C_lit

0.96

C_dup

C3 classification BC

Number of members (P>50%) 14

Radius (P>50% members) 11.9 [arcmin]

C_N 0.0 Sparse
C_dens 0.02 Very loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.96 Unique

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

Overview

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CWWDL 10428 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

Note: This is a unique object, which shares a very small percentage of members with at least one previously reported entry, and a very small percentage with at least one entry reported in the same catalogue. See table with shared members information.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=0.96) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 10428 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	–	359.001	63.312	0.299	-3.126	-1.095	-5.768
Chi et al.	2023	-1.073	63.355	0.307	-3.125	-1.053	-57.968

💡 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	–	–	–	66	0.120	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 11769	8.0	358.97	63.23	0.28	-2.85	-1.06	–	0.06
CWNU 2667	4.0	358.4	63.07	0.25	-3.25	-1.08	-78.56	0.59

💡 Note: The % column shows the percentage of members that CWWDL 10428 shares with each listed object.

Visualization

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