CWWDL 10434

0.06 UTI

0.38

C_N

0.26

C_dens

0.5

C_C3

0.0

C_lit

0.26

C_dup

C3 classification BB

Number of members (P>50%) 38

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

C_N 0.38 Poorly populated
C_dens 0.26 Loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.26 Possibly duplicate

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

Overview

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CWWDL 10434 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. It is catalogued as a metal-poor, very 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 Very young

Data

🔍 Search references for CWWDL 10434 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	–	353.004	61.994	0.32	-4.082	-1.426	-48.161
Chi et al.	2023	352.97	61.986	0.317	-4.041	-1.446	-48.161

💡 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	-0.580	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1185	73.7	353.1	62.13	0.32	-4.14	-1.29	-48.72	0.51

💡 Note: The % column shows the percentage of members that CWWDL 10434 shares with each listed object.

Visualization

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