CWNU 3535

0.07 UTI

0.51

C_N

0.46

C_dens

0.75

C_C3

0.0

C_lit

0.21

C_dup

C3 classification AB

Number of members (P>50%) 52

Radius (P>50% members) 2.0 [arcmin]

C_N 0.51 Moderately populated
C_dens 0.46 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.21 Likely duplicate

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

Overview

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CWNU 3535 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a large distance, well below the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Very distant Moderate extinction Intermediate age

Data

🔍 Search references for CWNU 3535 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	–	101.211	-9.436	0.122	0.005	0.767	83.188
He et al.	2023	101.208	-9.435	0.114	0.001	0.765	–

💡 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.	2023	7.08	1.65	–	158	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Juchert J0644.8-0925	78.8	101.21	-9.43	0.11	0.0	0.78	79.7	0.55

💡 Note: The % column shows the percentage of members that CWNU 3535 shares with each listed object.

Visualization

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