CWNU 3051

0.03 UTI

0.3

C_N

0.48

C_dens

0.25

C_C3

0.0

C_lit

0.13

C_dup

C3 classification CC

Number of members (P>50%) 30

Radius (P>50% members) 2.7 [arcmin]

C_N 0.3 Poorly populated
C_dens 0.48 Loose
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.13 Likely duplicate

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

Overview

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CWNU 3051 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age 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.

Distant Moderate extinction Intermediate age

Data

🔍 Search references for CWNU 3051 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	–	8.242	58.353	0.222	-2.535	-0.865	–
He et al.	2023	8.233	58.353	0.217	-2.555	-0.849	–

💡 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	3.72	2.10	–	631	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 960	86.7	8.23	58.35	0.22	-2.54	-0.86	–	0.41

💡 Note: The % column shows the percentage of members that CWNU 3051 shares with each listed object.

Visualization

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