CWNU 3065

0.11 UTI

0.55

C_N

0.03

C_dens

0.62

C_C3

0.0

C_lit

0.44

C_dup

N_m (P>50%) 59

Core radius and density 9.5 [pc], 0.1 [pc^-2]

C3 classification AC

C_N 0.55 Moderately populated
C_dens 0.03 Very loose
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.44 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 3065 is a moderately populated, very loose object of intermediate C3 quality. Its parallax locates it at a large distance, well 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 3065 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–	40.454	67.255	0.165	-0.878	0.344	-57.903
He et al.	2023	40.447	67.221	0.162	-0.853	0.356	-57.9

💡 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–	4.27	3.2	–	158	–	–	–	–
He et al.	2023	4.27	3.20	–	158	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1084	55.9	40.46	67.19	0.16	-0.87	0.34	-57.9	0.22

💡 Note: The % column shows the percentage of members that CWNU 3065 shares with each listed object.

Visualization

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