CWNU 3238

0.07 UTI

0.31

C_N

0.43

C_dens

0.75

C_C3

0.0

C_lit

0.23

C_dup

N₅₀ (P>50% members) 31

Stellar density (N₅₀/rad) 2.1 [N/pc²]

C3 classification AB

C_N 0.31 Poorly populated
C_dens 0.43 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.23 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 3238 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 young 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 Low extinction Young

Data

🔍 Search references for CWNU 3238 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–	340.202	50.892	0.873	-1.893	-4.131	-27.477
He et al.	2023	340.212	50.891	0.87	-1.902	-4.109	-21.86

💡 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–	1.12	0.55	–	79	–	–	–	–
He et al.	2023	1.12	0.55	–	79	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 801	77.4	340.2	50.89	0.88	-1.9	-4.11	-21.89	0.19

💡 Note: The % column shows the percentage of members that CWNU 3238 shares with each listed object.

Visualization

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