CWNU 465

0.00 UTI

0.56

C_N

1.0

C_dens

0.5

C_C3

0.0

C_lit

0.0

C_dup

C3 classification BB

Number of members (P>50%) 62

Radius (P>50% members) 3.8 [arcmin]

C_N 0.56 Moderately populated
C_dens 1.0 Very dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

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

Overview

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CWNU 465 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate^* distance, above the mid-plane, affected by high extinction. It is catalogued as a metal-rich, very young cluster (see Parameters). It is rarely studied 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, and a significant percentage with at least one entry reported in the same catalogue. See table with shared members information.

(*): The parallax distance estimate (~2.45 kpc) differs significantly from the median photometric distance (~4.79 kpc).

Distant High extinction Metal-rich Very young

Data

🔍 Search references for CWNU 465 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	–	83.641	37.237	0.408	0.915	-2.497	–
He et al.	2022	83.617	37.243	0.41	0.91	-2.5	–

💡 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.	2022	4.79	3.60	–	5	0.611	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1280	100.0	83.65	37.22	0.41	0.92	-2.49	26.19	0.55
CWWDL 12514	98.4	83.64	37.23	0.41	0.92	-2.49	–	0.0
CWNU 470	72.6	83.59	37.22	0.44	0.94	-2.48	26.41	0.13

💡 Note: The % column shows the percentage of members that CWNU 465 shares with each listed object.

Visualization

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