CWNU 3525

0.07 UTI

0.33

C_N

0.42

C_dens

0.5

C_C3

0.0

C_lit

0.27

C_dup

N₅₀ (P>50% members) 33

Stellar density (N₅₀/rad) 2.1 [N/pc²]

C3 classification BB

C_N 0.33 Poorly populated
C_dens 0.42 Loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.27 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 3525 is a poorly populated, loose object of intermediate 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 3525 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–	23.687	61.712	0.351	-1.42	-0.477	–
He et al.	2023	23.687	61.72	0.337	-1.42	-0.468	–

💡 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–	2.57	2.75	–	32	–	–	–	–
He et al.	2023	2.57	2.75	–	32	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1026	72.7	23.76	61.72	0.35	-1.42	-0.48	–	0.28

💡 Note: The % column shows the percentage of members that CWNU 3525 shares with each listed object.

Visualization

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