CWWDL 3527

0.05 UTI

0.0

C_N

0.2

C_dens

0.25

C_C3

0.0

C_lit

0.52

C_dup

C3 classification DB

Number of members (P>50%) 18

Radius (P>50% members) 4.2 [arcmin]

C_N 0.0 Sparse
C_dens 0.2 Very loose
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.52 Likely unique

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

Overview

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CWWDL 3527 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane. It is catalogued as a near-solar metallicity, 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.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 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	–	110.046	-21.385	0.287	-0.598	1.249	95.507
Chi et al.	2023	110.044	-21.389	0.298	-0.585	1.146	95.507

💡 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
Chi et al.	2023	–	–	–	54	0.420	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 2709	48.0	110.05	-21.41	0.29	-0.62	1.28	106.15	0.15

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

Visualization

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