CWNU 3386

0.24 UTI

0.37

C_N

0.07

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

N_m (P>50%) 37

Core radius and density 2.6 [pc], 0.3 [pc^-2]

C3 classification AB

C_N 0.37 Poorly populated
C_dens 0.07 Very loose
C_C3 0.75 High 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 3386 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a large^* distance, below the mid-plane, affected by low extinction. It is catalogued as an old cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~8.36 kpc) differs significantly from the median photometric distance (~5.50 kpc).

⚠️ 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 Low extinction Old

Data

🔍 Search references for CWNU 3386 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–	115.027	-30.657	0.12	-1.286	2.045	–
He et al.	2023	115.036	-30.657	0.13	-1.281	2.081	–

💡 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–	5.5	0.25	–	1585	–	–	–	–
He et al.	2023	5.50	0.25	–	1585	–	–	–	–

Visualization

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