CWNU 4433

0.08 UTI

0.25

C_N

0.27

C_dens

0.75

C_C3

0.0

C_lit

0.32

C_dup

C3 classification BA

Number of members (P>50%) 25

Radius (P>50% members) 3.1 [arcmin]

C_N 0.25 Poorly populated
C_dens 0.27 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.32 Possibly duplicate

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

Overview

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CWNU 4433 is a poorly populated, loose 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 an intermediate-age 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 High extinction Intermediate age

Data

🔍 Search references for CWNU 4433 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	–	281.246	-4.868	0.209	-1.581	-4.026	42.487
He et al.	2023	281.235	-4.873	0.21	-1.607	-3.985	35.71

💡 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	3.89	4.25	–	251	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 279	68.0	281.28	-4.86	0.21	-1.58	-4.07	42.49	0.27

💡 Note: The % column shows the percentage of members that CWNU 4433 shares with each listed object.

Visualization

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