CWNU 3264

0.18 UTI

0.62

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.37

C_dup

C3 classification AB

Number of members (P>50%) 75

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

C_N 0.62 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.37 Possibly duplicate

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

Overview

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CWNU 3264 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high 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 High extinction Intermediate age

Data

🔍 Search references for CWNU 3264 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	–	274.409	-16.361	0.299	-0.534	-1.046	41.111
He et al.	2023	274.409	-16.36	0.284	-0.546	-1.045	40.36

💡 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	2.69	4.70	–	158	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 178	62.7	274.41	-16.36	0.32	-0.53	-1.03	41.19	0.07
CWWDL 1713	56.0	274.41	-16.36	0.3	-0.53	-1.03	40.36	0.48

💡 Note: The % column shows the percentage of members that CWNU 3264 shares with each listed object.

Visualization

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