CWNU 3472

0.23 UTI

0.62

C_N

0.18

C_dens

0.75

C_C3

0.0

C_lit

0.73

C_dup

C3 classification AB

Number of members (P>50%) 75

Radius (P>50% members) 17.7 [arcmin]

C_N 0.62 Moderately populated
C_dens 0.18 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.73 Likely unique

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

Overview

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CWNU 3472 is a moderately populated, very loose object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as an intermediate-age 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 Low extinction Intermediate age

Data

🔍 Search references for CWNU 3472 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	–	128.154	-34.407	0.57	-4.53	3.293	9.148
He et al.	2023	128.135	-34.386	0.57	-4.556	3.284	–

💡 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	1.82	0.90	–	251	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 5431	26.7	128.42	-34.58	0.57	-4.55	3.29	32.9	0.15

💡 Note: The % column shows the percentage of members that CWNU 3472 shares with each listed object.

Visualization

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