CWNU 1065

0.35 UTI

0.33

C_N

0.65

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 33

Stellar density (N₅₀/rad) 3.2 [N/pc²]

C3 classification AB

C_N 0.33 Poorly populated
C_dens 0.65 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 1065 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Young

Data

🔍 Search references for CWNU 1065 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–	243.437	-51.255	0.82	0.161	-2.17	-12.485
Wei et al.	2025	243.5	-51.309	0.833	0.153	-2.156	–
He et al.	2022	243.489	-51.191	0.831	0.138	-2.159	–

💡 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–	1.56	1.44	–	85	-0.250	488	0.48	–
Wei et al.	2025	1.56	1.43	–	135	-0.250	488	0.48	–
He et al.	2022	–	1.45	–	35	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 2062	100.0	243.48	-51.28	0.82	0.16	-2.19	-11.47	0.19

💡 Note: The % column shows the percentage of members that CWNU 1065 shares with each listed object.

Visualization

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