CWNU 479

0.07 UTI

0.27

C_N

0.24

C_dens

0.38

C_C3

0.0

C_lit

0.41

C_dup

C3 classification CB

Number of members (P>50%) 27

Radius (P>50% members) 9.2 [arcmin]

C_N 0.27 Poorly populated
C_dens 0.24 Very loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.41 Possibly duplicate

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

Overview

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CWNU 479 is a poorly populated, very loose object of low 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-rich, very young cluster (see Parameters). It is rarely studied in the literature.

⚠️ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Low extinction Metal-rich Very young

Data

🔍 Search references for CWNU 479 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	–	5.23	52.587	0.561	-2.053	-1.355	-37.293
He et al.	2022	5.224	52.613	0.57	-2.11	-1.41	–

💡 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	2.29	0.84	–	10	0.805	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1197	59.3	5.36	52.69	0.55	-2.02	-1.35	-37.29	0.12
Theia 2936	7.4	6.1	52.74	0.57	-1.99	-1.32	-37.72	0.01

💡 Note: The % column shows the percentage of members that CWNU 479 shares with each listed object.

Visualization

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