CWNU 3786

0.20 UTI

0.43

C_N

0.22

C_dens

0.38

C_C3

0.0

C_lit

1.0

C_dup

N_m (P>50%) 43

Core radius and density 2.0 [pc], 1.1 [pc^-2]

C3 classification BC

C_N 0.43 Poorly populated
C_dens 0.22 Very loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 3786 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as an old cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Very distant Moderate extinction Old

Data

🔍 Search references for CWNU 3786 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–	106.223	-9.514	0.164	-0.596	0.895	49.739
He et al.	2023	106.223	-9.511	0.185	-0.586	0.909	49.74

💡 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–	5.01	2.95	–	1585	–	–	–	–
He et al.	2023	5.01	2.95	–	1585	–	–	–	–

Visualization

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