CWWDL 2965

0.11 UTI

0.4

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.25

C_dup

C3 classification AB

Number of members (P>50%) 40

Radius (P>50% members) 2.0 [arcmin]

C_N 0.4 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.25 Possibly duplicate

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

Overview

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CWWDL 2965 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, 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 2965 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	–	107.727	-3.43	0.235	-0.351	0.06	63.802
Chi et al.	2023	107.731	-3.432	0.259	-0.476	0.118	62.491

💡 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	–	–	–	214	-0.880	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1351	75.0	107.73	-3.42	0.23	-0.34	0.02	63.8	0.64

💡 Note: The % column shows the percentage of members that CWWDL 2965 shares with each listed object.

Visualization

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