CWWDL 566

0.08 UTI

0.62

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.15

C_dup

C3 classification AA

Number of members (P>50%) 75

Radius (P>50% members) 4.0 [arcmin]

C_N 0.62 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.15 Likely duplicate

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

Overview

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CWWDL 566 is a moderately populated, very dense object of very high 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.

⚠️ Warning: This is likely a duplicate object, which shares a large 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 566 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	–	316.051	42.059	0.483	-2.435	-4.328	-17.431
Chi et al.	2023	316.046	42.065	0.485	-2.458	-4.396	-12.543

💡 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	–	–	–	29	0.370	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FoF 876	85.3	316.06	42.06	0.48	-2.44	-4.32	-17.43	0.69
UBC 145	77.3	316.06	42.07	0.48	-2.44	-4.31	-17.43	0.0

💡 Note: The % column shows the percentage of members that CWWDL 566 shares with each listed object.

Visualization

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