CWNU 2965

0.05 UTI

0.33

C_N

0.39

C_dens

0.38

C_C3

0.0

C_lit

0.24

C_dup

C3 classification BC

Number of members (P>50%) 33

Radius (P>50% members) 5.0 [arcmin]

C_N 0.33 Poorly populated
C_dens 0.39 Loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.24 Likely duplicate

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

Overview

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CWNU 2965 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a young cluster (see Parameters). It was recently reported in the literature.

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

Relatively close Moderate extinction Young

Data

🔍 Search references for CWNU 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	–	98.337	6.234	0.356	-0.506	-2.795	–
He et al.	2023	98.344	6.238	0.348	-0.492	-2.795	–

💡 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
He et al.	2023	2.45	1.95	–	32	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1615	75.8	98.35	6.23	0.34	-0.5	-2.8	–	0.25

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

Visualization

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