CWNU 3527

0.16 UTI

0.57

C_N

0.58

C_dens

0.38

C_C3

0.0

C_lit

0.54

C_dup

C3 classification CB

Number of members (P>50%) 65

Radius (P>50% members) 4.7 [arcmin]

C_N 0.57 Moderately populated
C_dens 0.58 Moderately dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.54 Likely unique

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

Overview

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CWNU 3527 is a moderately populated, moderately dense 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 an intermediate-age 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.

Relatively close High extinction Intermediate age

Data

🔍 Search references for CWNU 3527 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	–	279.867	-5.349	0.289	0.239	-2.191	131.378
He et al.	2023	279.867	-5.356	0.294	0.24	-2.2	88.61

💡 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	2.88	4.20	–	100	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 265	46.2	279.86	-5.35	0.29	0.24	-2.2	131.38	0.3

💡 Note: The % column shows the percentage of members that CWNU 3527 shares with each listed object.

Visualization

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