CWNU 3560

0.12 UTI

0.46

C_N

0.05

C_dens

0.75

C_C3

0.0

C_lit

0.48

C_dup

N_m (P>50%) 46

Core radius and density 2.6 [pc], 0.2 [pc^-2]

C3 classification AB

C_N 0.46 Poorly populated
C_dens 0.05 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.48 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 3560 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a young 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 Moderate extinction Young

Data

🔍 Search references for CWNU 3560 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–	118.626	-28.213	0.325	-2.825	3.076	–
He et al.	2023	118.63	-28.227	0.325	-2.835	3.082	–

💡 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–	2.69	1.3	–	20	–	–	–	–
He et al.	2023	2.69	1.30	–	20	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 4356	52.2	118.61	-28.3	0.33	-2.81	3.08	57.29	0.18

💡 Note: The % column shows the percentage of members that CWNU 3560 shares with each listed object.

Visualization

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