CWNU 3208

0.02 UTI

0.31

C_N

0.27

C_dens

0.75

C_C3

0.0

C_lit

0.06

C_dup

C3 classification AB

Number of members (P>50%) 31

Radius (P>50% members) 2.9 [arcmin]

C_N 0.31 Poorly populated
C_dens 0.27 Loose
C_C3 0.75 High 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 3208 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by high extinction. It is catalogued as a 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.

Very distant High extinction Young

Data

🔍 Search references for CWNU 3208 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	–	131.613	-50.83	0.177	-4.718	4.846	–
He et al.	2023	131.596	-50.834	0.189	-4.727	4.846	–

💡 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	6.17	3.85	–	50	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2181	93.5	131.61	-50.83	0.19	-4.73	4.85	–	0.39

💡 Note: The % column shows the percentage of members that CWNU 3208 shares with each listed object.

Visualization

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