CWWDL 58

0.01 UTI

0.48

C_N

0.81

C_dens

0.62

C_C3

0.0

C_lit

0.02

C_dup

C3 classification CA

Number of members (P>50%) 48

Radius (P>50% members) 3.9 [arcmin]

C_N 0.48 Poorly populated
C_dens 0.81 Dense
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.02 Very likely duplicate

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

Overview

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CWWDL 58 is a poorly populated, dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Near-solar metallicity Intermediate age

Data

🔍 Search references for CWWDL 58 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	–	332.933	45.18	0.33	-4.243	-4.969	-48.048
Chi et al.	2023	332.942	45.179	0.33	-4.27	-4.942	-50.106

💡 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	–	–	–	427	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1142	97.9	332.92	45.17	0.33	-4.25	-4.96	-48.29	0.51

💡 Note: The % column shows the percentage of members that CWWDL 58 shares with each listed object.

Visualization

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