CWNU 4188

0.08 UTI

0.34

C_N

0.12

C_dens

0.38

C_C3

0.0

C_lit

0.47

C_dup

C3 classification BC

Number of members (P>50%) 34

Radius (P>50% members) 5.5 [arcmin]

C_N 0.34 Poorly populated
C_dens 0.12 Very loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.47 Possibly duplicate

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

Overview

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CWNU 4188 is a poorly populated, very 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 young cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Distant Moderate extinction Young

Data

🔍 Search references for CWNU 4188 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	–	115.17	-25.321	0.209	-1.991	3.219	73.725
He et al.	2023	115.134	-25.294	0.21	-1.978	3.237	73.73

💡 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	4.27	1.75	–	40	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1926	52.9	115.21	-25.33	0.21	-2.0	3.21	73.73	0.1

💡 Note: The % column shows the percentage of members that CWNU 4188 shares with each listed object.

Visualization

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