CWNU 3508

0.10 UTI

0.37

C_N

1.0

C_dens

0.38

C_C3

0.0

C_lit

0.3

C_dup

C3 classification CB

Number of members (P>50%) 37

Radius (P>50% members) 1.3 [arcmin]

C_N 0.37 Poorly populated
C_dens 1.0 Very dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.3 Possibly duplicate

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

Overview

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CWNU 3508 is a poorly populated, very 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 possibly a duplicate object, which shares a significant 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 3508 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	–	155.09	-58.633	0.248	-5.49	2.818	28.653
He et al.	2023	155.091	-58.64	0.242	-5.472	2.806	28.65

💡 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	3.47	2.20	–	501	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2334	70.3	155.1	-58.64	0.25	-5.48	2.82	28.65	0.35

💡 Note: The % column shows the percentage of members that CWNU 3508 shares with each listed object.

Visualization

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