CWNU 3340

0.09 UTI

0.5

C_N

0.5

C_dens

0.38

C_C3

0.0

C_lit

0.32

C_dup

C3 classification CB

Number of members (P>50%) 50

Radius (P>50% members) 7.9 [arcmin]

C_N 0.5 Moderately populated
C_dens 0.5 Moderately dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.32 Possibly duplicate

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

Overview

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CWNU 3340 is a moderately populated, moderately dense object of low C3 quality. Its parallax locates it at a relatively close distance, near 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.

Relatively close Moderate extinction Intermediate age

Data

🔍 Search references for CWNU 3340 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	–	93.023	16.224	0.514	-0.014	-3.045	-5.452
He et al.	2023	93.024	16.23	0.518	-0.012	-3.045	-5.61

💡 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	3.00	–	158	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1538	68.0	93.02	16.22	0.51	-0.01	-3.04	-5.53	0.32

💡 Note: The % column shows the percentage of members that CWNU 3340 shares with each listed object.

Visualization

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