CWNU 3582

0.08 UTI

0.38

C_N

0.65

C_dens

0.75

C_C3

0.0

C_lit

0.24

C_dup

C3 classification AB

Number of members (P>50%) 38

Radius (P>50% members) 7.8 [arcmin]

C_N 0.38 Poorly populated
C_dens 0.65 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.24 Likely duplicate

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

Overview

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CWNU 3582 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is 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 Intermediate age

Data

🔍 Search references for CWNU 3582 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	–	249.571	-52.463	0.662	-2.003	-1.626	-18.95
He et al.	2023	249.566	-52.47	0.663	-2.003	-1.617	-19.07

💡 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	1.48	1.85	–	251	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2764	76.3	249.58	-52.46	0.66	-2.0	-1.63	-18.5	0.34

💡 Note: The % column shows the percentage of members that CWNU 3582 shares with each listed object.

Visualization

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