CWNU 3324

0.01 UTI

0.33

C_N

1.0

C_dens

0.25

C_C3

0.0

C_lit

0.03

C_dup

C3 classification DB

Number of members (P>50%) 33

Radius (P>50% members) 4.0 [arcmin]

C_N 0.33 Poorly populated
C_dens 1.0 Very dense
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.03 Very likely duplicate

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

Overview

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CWNU 3324 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a very young 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.

Relatively close High extinction Very young

Data

🔍 Search references for CWNU 3324 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	–	39.021	60.31	0.461	0.12	-0.774	–
He et al.	2023	39.013	60.308	0.468	0.121	-0.774	–

💡 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	1.91	3.20	–	16	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1106	97.0	38.99	60.31	0.46	0.13	-0.77	–	0.3

💡 Note: The % column shows the percentage of members that CWNU 3324 shares with each listed object.

Visualization

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