CWNU 3086

0.10 UTI

0.26

C_N

0.07

C_dens

0.62

C_C3

0.0

C_lit

0.54

C_dup

N₅₀ (P>50% members) 26

Stellar density (N₅₀/rad) 0.3 [N/pc²]

C3 classification AC

C_N 0.26 Poorly populated
C_dens 0.07 Very loose
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.54 Likely unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 3086 is a poorly populated, very loose object of intermediate 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.

Note: This is likely a unique object, which shares a moderate 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 3086 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–	103.643	-19.303	0.347	-0.914	3.374	–
He et al.	2023	103.62	-19.395	0.324	-0.908	3.378	42.49

💡 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–	2.75	1.05	–	79	–	–	–	–
He et al.	2023	2.75	1.05	–	79	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1826	46.2	103.66	-19.56	0.33	-0.94	3.39	–	0.06

💡 Note: The % column shows the percentage of members that CWNU 3086 shares with each listed object.

Visualization

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