CWNU 213

0.41 UTI

0.42

C_N

0.88

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 42

Radius (P>50% members) 7.5 [arcmin]

C_N 0.42 Poorly populated
C_dens 0.88 Dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

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CWNU 213 is a poorly populated, dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old cluster (see Parameters). It is rarely studied in the literature.

Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Old

Data

🔍 Search references for CWNU 213 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	–	319.804	56.981	0.706	3.542	0.191	-27.084
He et al.	2022	319.783	56.954	0.7	3.53	0.19	-26.8

💡 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.	2022	1.10	2.34	–	1585	0.169	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 7580	100.0	319.8	56.99	0.71	3.53	0.2	-27.08	0.11
CWWDL 14235	83.3	319.81	56.98	0.71	3.55	0.19	-27.08	0.0

💡 Note: The % column shows the percentage of members that CWNU 213 shares with each listed object.

Visualization

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