CWNU 3192

0.04 UTI

0.26

C_N

0.43

C_dens

0.25

C_C3

0.0

C_lit

0.19

C_dup

N₅₀ (P>50% members) 26

Stellar density (N₅₀/rad) 2.1 [N/pc²]

C3 classification DB

C_N 0.26 Poorly populated
C_dens 0.43 Loose
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.19 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 3192 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a moderate distance, below 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 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 3192 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–	113.168	-23.857	0.392	-2.656	3.155	–
He et al.	2023	113.15	-23.848	0.388	-2.651	3.161	–

💡 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–	2.4	1.75	–	13	–	–	–	–
He et al.	2023	2.40	1.75	–	13	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1906	80.8	113.09	-23.84	0.39	-2.65	3.17	–	0.24

💡 Note: The % column shows the percentage of members that CWNU 3192 shares with each listed object.

Visualization

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