CWNU 3365

0.21 UTI

0.76

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.42

C_dup

C3 classification AB

Number of members (P>50%) 132

Radius (P>50% members) 4.7 [arcmin]

C_N 0.76 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.42 Possibly duplicate

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

Overview

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CWNU 3365 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above 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.

Distant High extinction Intermediate age

Data

🔍 Search references for CWNU 3365 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	–	343.44	62.813	0.268	-1.991	-1.022	-56.862
He et al.	2023	343.418	62.817	0.27	-1.99	-1.008	-56.86

💡 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	3.02	3.60	–	158	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 868	57.6	343.42	62.81	0.27	-1.98	-1.01	-56.86	0.32
FoF 1822	22.0	343.41	62.82	0.26	-2.11	-1.01	-101.64	0.28

💡 Note: The % column shows the percentage of members that CWNU 3365 shares with each listed object.

Visualization

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