CWNU 341

0.01 UTI

0.75

C_N

1.0

C_dens

0.38

C_C3

0.0

C_lit

0.02

C_dup

N₅₀ (P>50% members) 100

Stellar density (N₅₀/rad) 10.2 [N/pc²]

C3 classification CB

C_N 0.75 Rich
C_dens 1.0 Very dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.02 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWNU 341 is a rich, very dense 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 metal-rich, old cluster (see Parameters). It is rarely studied in the literature.

⚠️ Warning: This is very 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 Metal-rich Old

Data

🔍 Search references for CWNU 341 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	99999–	111.13	-17.191	0.344	-1.35	-0.5	40.335
He et al.	2022	111.135	-17.191	0.34	-1.33	-0.49	41.3

💡 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]	B_frac	BSS
UCC	99999–	2.29	1.32	–	1000	0.680	–	–	–
He et al.	2022	2.29	1.32	–	1000	0.680	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1371	98.0	111.13	-17.19	0.34	-1.35	-0.49	32.63	0.57

💡 Note: The % column shows the percentage of members that CWNU 341 shares with each listed object.

Visualization

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