CWNU 306

0.01 UTI

0.32

C_N

0.33

C_dens

0.75

C_C3

0.0

C_lit

0.03

C_dup

N_m (P>50%) 32

Core radius and density 1.2 [pc], 1.6 [pc^-2]

C3 classification AB

C_N 0.32 Poorly populated
C_dens 0.33 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.03 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 306 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a metal-poor, very young 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-poor Very young

Data

🔍 Search references for CWNU 306 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–	119.952	-45.576	0.614	-3.496	5.027	38.205
He et al.	2022	119.998	-45.549	0.61	-3.53	5.0	–

💡 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–	1.26	0.57	–	10	-0.580	–	–	–
He et al.	2022	1.26	0.57	–	10	-0.580	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1619	96.9	119.95	-45.58	0.61	-3.5	5.03	20.06	0.33

💡 Note: The % column shows the percentage of members that CWNU 306 shares with each listed object.

Visualization

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