CWWDL 9622

0.01 UTI

0.37

C_N

1.0

C_dens

0.62

C_C3

0.0

C_lit

0.03

C_dup

C3 classification CA

Number of members (P>50%) 37

Radius (P>50% members) 2.3 [arcmin]

C_N 0.37 Poorly populated
C_dens 1.0 Very dense
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.03 Very likely duplicate

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

Overview

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CWWDL 9622 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near 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 very 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 Very young

Data

🔍 Search references for CWWDL 9622 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	–	224.489	-58.057	0.419	-4.865	-2.939	-49.695
Chi et al.	2023	224.48	-58.053	0.421	-4.879	-2.984	-49.695

💡 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	–	–	–	1	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 1528	97.3	224.49	-58.06	0.42	-4.86	-2.91	-49.7	0.52

💡 Note: The % column shows the percentage of members that CWWDL 9622 shares with each listed object.

Visualization

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