CWNU 3323

0.01 UTI

0.28

C_N

0.24

C_dens

0.25

C_C3

0.0

C_lit

0.07

C_dup

N₅₀ (P>50% members) 28

Stellar density (N₅₀/rad) 1.2 [N/pc²]

C3 classification CC

C_N 0.28 Poorly populated
C_dens 0.24 Very loose
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.07 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWNU 3323 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a large^* distance, above 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.

(*): The parallax distance estimate (~6.68 kpc) differs significantly from the median photometric distance (~15.14 kpc).

Extremely distant High extinction Very young

Data

🔍 Search references for CWNU 3323 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	99999–	336.136	60.414	0.15	-2.325	-1.283	–
He et al.	2023	336.134	60.414	0.113	-2.323	-1.307	–

💡 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]	B_frac	BSS
UCC	99999–	15.14	5.0	–	1	–	–	–	–
He et al.	2023	15.14	5.00	–	1	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Teutsch 53	92.9	336.14	60.41	0.15	-2.32	-1.33	–	0.31

💡 Note: The % column shows the percentage of members that CWNU 3323 shares with each listed object.

Visualization

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