CWWDL 3133

0.00 UTI

0.46

C_N

1.0

C_dens

0.62

C_C3

0.0

C_lit

0.0

C_dup

C3 classification CA

Number of members (P>50%) 46

Radius (P>50% members) 2.2 [arcmin]

C_N 0.46 Poorly populated
C_dens 1.0 Very dense
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

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

Overview

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CWWDL 3133 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above 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 3133 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	–	60.228	59.2	0.374	-1.827	-1.38	-14.679
Chi et al.	2023	60.238	59.193	0.397	-1.845	-1.386	-21.177

💡 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	–	–	–	174	-0.100	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
LISC 3058	100.0	60.21	59.19	0.38	-1.82	-1.38	-14.68	0.0
UBC 49	100.0	60.22	59.19	0.38	-1.82	-1.38	-14.68	0.7
OC 0269	78.3	60.23	59.2	0.38	-1.82	-1.38	-14.68	0.0

💡 Note: The % column shows the percentage of members that CWWDL 3133 shares with each listed object.

Visualization

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