CWNU 4126

0.17 UTI

0.47

C_N

0.33

C_dens

0.5

C_C3

0.0

C_lit

0.64

C_dup

C3 classification BB

Number of members (P>50%) 47

Radius (P>50% members) 6.4 [arcmin]

C_N 0.47 Poorly populated
C_dens 0.33 Loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.64 Likely unique

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

Overview

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CWNU 4126 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a young cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate extinction Young

Data

🔍 Search references for CWNU 4126 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	–	246.136	-48.794	0.349	-1.275	-2.783	-32.711
He et al.	2023	246.135	-48.794	0.357	-1.293	-2.769	-32.71

💡 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	2.40	2.75	–	20	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2776	36.2	246.06	-48.86	0.36	-1.36	-2.85	-34.7	0.16

💡 Note: The % column shows the percentage of members that CWNU 4126 shares with each listed object.

Visualization

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