CWNU 3528

0.14 UTI

0.6

C_N

0.19

C_dens

0.38

C_C3

0.0

C_lit

0.61

C_dup

C3 classification BC

Number of members (P>50%) 70

Radius (P>50% members) 8.8 [arcmin]

C_N 0.6 Moderately populated
C_dens 0.19 Very loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.61 Likely unique

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

Overview

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CWNU 3528 is a moderately populated, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a young cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Distant High extinction Young

Data

🔍 Search references for CWNU 3528 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	–	68.832	47.157	0.301	-0.393	-0.938	-67.275
He et al.	2023	68.886	47.144	0.3	-0.382	-0.938	–

💡 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	3.55	4.35	–	50	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1246	38.6	68.84	47.13	0.3	-0.4	-0.95	–	0.16

💡 Note: The % column shows the percentage of members that CWNU 3528 shares with each listed object.

Visualization

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