CWNU 3358

0.02 UTI

0.33

C_N

0.69

C_dens

0.25

C_C3

0.0

C_lit

0.06

C_dup

C3 classification DB

Number of members (P>50%) 33

Radius (P>50% members) 2.3 [arcmin]

C_N 0.33 Poorly populated
C_dens 0.69 Moderately dense
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.06 Very likely duplicate

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

Overview

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CWNU 3358 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported in the literature.

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

Distant Moderate extinction Intermediate age

Data

🔍 Search references for CWNU 3358 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	–	147.152	-58.669	0.216	-5.21	3.591	21.473
He et al.	2023	147.15	-58.669	0.216	-5.183	3.591	31.12

💡 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	3.89	2.20	–	501	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2294	93.9	147.16	-58.67	0.21	-5.2	3.59	21.47	0.09
CWWDL 208	75.8	147.15	-58.67	0.23	-5.24	3.59	22.65	0.33

💡 Note: The % column shows the percentage of members that CWNU 3358 shares with each listed object.

Visualization

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