CWNU 424

0.05 UTI

0.26

C_N

0.73

C_dens

0.25

C_C3

0.0

C_lit

0.19

C_dup

C3 classification DB

Number of members (P>50%) 26

Radius (P>50% members) 6.7 [arcmin]

C_N 0.26 Poorly populated
C_dens 0.73 Moderately dense
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.19 Likely duplicate

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

Overview

ℹ️

CWNU 424 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

⚠️ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for CWNU 424 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	74.407	32.776	0.729	2.316	-5.737	6.824
He et al.	2022	74.411	32.774	0.74	2.31	-5.73	7.6

💡 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	1.26	2.64	–	251	0.051	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0289	80.8	74.36	32.77	0.73	2.35	-5.76	7.06	0.32

💡 Note: The % column shows the percentage of members that CWNU 424 shares with each listed object.

Visualization

ℹ️