CWWDL 65

0.07 UTI

0.0

C_N

0.52

C_dens

0.5

C_C3

0.0

C_lit

0.32

C_dup

C3 classification BB

Number of members (P>50%) 21

Radius (P>50% members) 2.9 [arcmin]

C_N 0.0 Sparse
C_dens 0.52 Moderately dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.32 Possibly duplicate

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

Overview

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CWWDL 65 is a sparse, moderately 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 possibly a duplicate object, which shares a significant 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 65 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	–	98.657	-6.839	0.297	0.281	0.174	30.883
Chi et al.	2023	98.651	-6.805	0.301	0.271	0.336	34.713

💡 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	-0.280	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 443	68.0	98.64	-6.83	0.29	0.27	0.08	27.98	0.68

💡 Note: The % column shows the percentage of members that CWWDL 65 shares with each listed object.

Visualization

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