CWWDL 10426

0.11 UTI

0.36

C_N

0.05

C_dens

0.38

C_C3

0.0

C_lit

0.72

C_dup

C3 classification CB

Number of members (P>50%) 36

Radius (P>50% members) 13.9 [arcmin]

C_N 0.36 Poorly populated
C_dens 0.05 Very loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.72 Likely unique

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

Overview

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CWWDL 10426 is a poorly populated, 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, very young cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate 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 10426 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	–	357.547	62.972	0.321	-3.036	-1.364	-89.175
Chi et al.	2023	357.738	62.91	0.32	-3.082	-1.357	-82.82

💡 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	–	–	–	18	0.270	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Teutsch 23	27.8	356.95	63.05	0.31	-2.97	-1.4	-66.91	0.84
Negueruela 1	8.3	356.86	63.21	0.31	-2.97	-1.38	–	0.85
King 21	5.6	357.49	62.7	0.32	-3.24	-1.71	-78.27	0.91

💡 Note: The % column shows the percentage of members that CWWDL 10426 shares with each listed object.

Visualization

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