CWNU 365

0.02 UTI

0.52

C_N

0.45

C_dens

0.5

C_C3

0.0

C_lit

0.07

C_dup

C3 classification BB

Number of members (P>50%) 55

Radius (P>50% members) 5.7 [arcmin]

C_N 0.52 Moderately populated
C_dens 0.45 Loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.07 Very likely duplicate

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

Overview

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CWNU 365 is a moderately populated, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by low 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 Low extinction Metal-rich Old

Data

🔍 Search references for CWNU 365 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	–	45.496	47.963	0.334	0.523	-1.236	-28.277
He et al.	2022	45.503	47.966	0.33	0.49	-1.24	-30.1

💡 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.	2022	2.75	0.54	–	1585	0.916	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1246	92.7	45.48	47.96	0.34	0.53	-1.24	-28.68	0.45
OC 0268	43.6	45.49	47.94	0.35	0.51	-1.25	-28.68	0.0

💡 Note: The % column shows the percentage of members that CWNU 365 shares with each listed object.

Visualization

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