CWNU 4472

0.16 UTI

0.34

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.38

C_dup

C3 classification AB

Number of members (P>50%) 34

Radius (P>50% members) 3.5 [arcmin]

C_N 0.34 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.38 Possibly duplicate

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

Overview

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CWNU 4472 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by low extinction. It is catalogued as a very 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.

Close Low extinction Very young

Data

🔍 Search references for CWNU 4472 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	–	325.137	58.224	1.066	-2.023	-3.195	58.044
He et al.	2023	325.114	58.223	1.068	-2.012	-3.189	58.04

💡 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	0.89	0.05	–	1	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 14476	61.8	325.15	58.19	1.06	-2.03	-3.38	-7.2	0.38

💡 Note: The % column shows the percentage of members that CWNU 4472 shares with each listed object.

Visualization

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