CWNU 4212

0.32 UTI

0.3

C_N

0.99

C_dens

0.38

C_C3

0.0

C_lit

0.97

C_dup

C3 classification CB

Number of members (P>50%) 30

Radius (P>50% members) 1.8 [arcmin]

C_N 0.3 Poorly populated
C_dens 0.99 Very dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.97 Unique

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

Overview

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CWNU 4212 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as an old cluster (see Parameters). It was recently reported in the literature.

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

Distant Moderate extinction Old

Data

🔍 Search references for CWNU 4212 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	–	91.982	26.598	0.213	0.463	-1.782	20.543
He et al.	2023	91.98	26.596	0.23	0.424	-1.749	20.54

💡 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	4.79	1.30	–	1259	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FoF 1374	3.3	91.67	26.5	0.27	0.16	-1.67	55.48	0.05

💡 Note: The % column shows the percentage of members that CWNU 4212 shares with each listed object.

Visualization

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