CWWDL 532

0.14 UTI

0.61

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.31

C_dup

C3 classification AB

Number of members (P>50%) 72

Radius (P>50% members) 4.9 [arcmin]

C_N 0.61 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.31 Possibly duplicate

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

Overview

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CWWDL 532 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate 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.

⚠️ Warning: This is possibly a duplicate object, which shares a significant 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 532 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	–	178.102	-64.603	0.419	-5.6	0.288	-24.15
Chi et al.	2023	178.168	-64.597	0.413	-5.602	0.287	-18.533

💡 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	–	–	–	13	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0575	69.4	178.1	-64.6	0.41	-5.6	0.29	-26.92	0.17
UBC 281	54.2	178.18	-64.6	0.41	-5.6	0.26	-29.69	0.65

💡 Note: The % column shows the percentage of members that CWWDL 532 shares with each listed object.

Visualization

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