CWNU 3580

0.02 UTI

0.31

C_N

0.53

C_dens

0.38

C_C3

0.0

C_lit

0.06

C_dup

C3 classification CB

Number of members (P>50%) 31

Radius (P>50% members) 9.4 [arcmin]

C_N 0.31 Poorly populated
C_dens 0.53 Moderately dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.06 Very likely duplicate

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

Overview

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CWNU 3580 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a very young cluster (see Parameters). It was recently reported 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 Moderate extinction Very young

Data

🔍 Search references for CWNU 3580 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	–	259.723	-33.574	0.802	2.366	-1.831	55.595
He et al.	2023	259.721	-33.56	0.811	2.363	-1.834	–

💡 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.	2023	1.17	1.60	–	16	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2914	93.5	259.72	-33.55	0.8	2.36	-1.84	55.59	0.21

💡 Note: The % column shows the percentage of members that CWNU 3580 shares with each listed object.

Visualization

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