CWWDL 3218

0.11 UTI

0.68

C_N

0.67

C_dens

0.75

C_C3

0.0

C_lit

0.27

C_dup

C3 classification AB

Number of members (P>50%) 86

Radius (P>50% members) 4.1 [arcmin]

C_N 0.68 Moderately populated
C_dens 0.67 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.27 Possibly duplicate

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

Overview

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CWWDL 3218 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, well above the mid-plane. It is catalogued as a metal-poor, intermediate-age 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 Intermediate age

Data

🔍 Search references for CWWDL 3218 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	–	71.689	60.873	0.236	0.552	-0.102	-18.761
Chi et al.	2023	71.712	60.873	0.259	0.542	-0.099	-23.002

💡 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	–	–	–	200	-0.580	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 3067	80.2	71.69	60.88	0.23	0.55	-0.1	-18.76	0.01
CWWL 3078	73.3	71.69	60.88	0.23	0.55	-0.1	-18.76	0.62

💡 Note: The % column shows the percentage of members that CWWDL 3218 shares with each listed object.

Visualization

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