CWNU 4043

0.06 UTI

0.4

C_N

0.51

C_dens

0.75

C_C3

0.0

C_lit

0.18

C_dup

C3 classification BA

Number of members (P>50%) 40

Radius (P>50% members) 3.2 [arcmin]

C_N 0.4 Poorly populated
C_dens 0.51 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.18 Likely duplicate

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

Overview

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CWNU 4043 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, near 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 likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Distant High extinction Young

Data

🔍 Search references for CWNU 4043 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	–	280.25	-5.634	0.236	-1.249	-3.145	52.191
He et al.	2023	280.252	-5.623	0.24	-1.25	-3.155	51.86

💡 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]	Bfr	BSS
He et al.	2023	3.39	4.85	–	32	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 262	82.5	280.25	-5.65	0.22	-1.23	-3.12	52.83	0.36

💡 Note: The % column shows the percentage of members that CWNU 4043 shares with each listed object.

Visualization

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