CWNU 3435

0.05 UTI

0.3

C_N

0.16

C_dens

0.75

C_C3

0.0

C_lit

0.2

C_dup

C3 classification AB

Number of members (P>50%) 30

Radius (P>50% members) 5.7 [arcmin]

C_N 0.3 Poorly populated
C_dens 0.16 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.2 Likely duplicate

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

Overview

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CWNU 3435 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high 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.

Distant High extinction Intermediate age

Data

🔍 Search references for CWNU 3435 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	–	11.135	63.782	0.27	0.288	-0.609	-29.022
He et al.	2023	11.092	63.781	0.27	0.295	-0.602	-29.02

💡 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	3.16	3.45	–	251	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 975	80.0	11.17	63.78	0.27	0.28	-0.61	-29.02	0.13

💡 Note: The % column shows the percentage of members that CWNU 3435 shares with each listed object.

Visualization

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