CWWDL 529

0.12 UTI

0.0

C_N

0.29

C_dens

0.75

C_C3

0.0

C_lit

0.56

C_dup

C3 classification AB

Number of members (P>50%) 17

Radius (P>50% members) 6.2 [arcmin]

C_N 0.0 Sparse
C_dens 0.29 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.56 Likely unique

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

Overview

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CWWDL 529 is a sparse, loose object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane. It is catalogued as a near-solar metallicity, very 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 Very young

Data

🔍 Search references for CWWDL 529 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	–	166.761	-62.833	0.528	-7.0	1.845	-17.772
Chi et al.	2023	166.761	-62.859	0.543	-6.999	1.896	-17.772

💡 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	–	–	–	3	-0.100	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 269	44.0	166.78	-62.87	0.55	-7.04	1.7	-17.77	0.61

💡 Note: The % column shows the percentage of members that CWWDL 529 shares with each listed object.

Visualization

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