CWNU 3684

0.17 UTI

0.55

C_N

1.0

C_dens

0.38

C_C3

0.0

C_lit

0.45

C_dup

C3 classification CB

Number of members (P>50%) 60

Radius (P>50% members) 1.4 [arcmin]

C_N 0.55 Moderately populated
C_dens 1.0 Very dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.45 Possibly duplicate

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

Overview

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CWNU 3684 is a moderately populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by low extinction. It is catalogued as a very young 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 Low extinction Very young

Data

🔍 Search references for CWNU 3684 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	–	158.742	-59.638	0.218	-5.481	2.38	16.279
He et al.	2023	158.762	-59.634	0.21	-5.482	2.378	–

💡 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	4.90	0.75	–	2	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2354	55.0	158.75	-59.63	0.21	-5.5	2.4	16.28	0.37

💡 Note: The % column shows the percentage of members that CWNU 3684 shares with each listed object.

Visualization

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