CWNU 4051

0.08 UTI

0.31

C_N

0.8

C_dens

0.75

C_C3

0.0

C_lit

0.23

C_dup

C3 classification AB

Number of members (P>50%) 31

Radius (P>50% members) 3.3 [arcmin]

C_N 0.31 Poorly populated
C_dens 0.8 Dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.23 Likely duplicate

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

Overview

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CWNU 4051 is a poorly populated, dense object of high C3 quality. Its parallax locates it at a moderate distance, below 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 4051 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	–	26.175	56.114	0.345	-0.894	-1.03	–
He et al.	2023	26.201	56.105	0.323	-0.916	-1.019	–

💡 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	2.82	1.10	–	32	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1055	77.4	26.18	56.11	0.33	-0.89	-1.03	–	0.43

💡 Note: The % column shows the percentage of members that CWNU 4051 shares with each listed object.

Visualization

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